OGLE-ing the Magellanic System : Cepheids in the Bridge

We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical perio...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Jacyszyn-Dobrzeniecka, Anna M. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020 January 22

Anmerkung:	Gesehen am 17.02.2020
Umfang:	16

Übergeordnetes Werk:	Enthalten in: The astrophysical journal - London : Institute of Physics Publ., 1995, 889(2020,1) Artikel-Nummer 25, 16 Seiten
Übergeordnetes Werk:	volume:889 ; year:2020 ; pages:25 ; extent:16

Links:	Volltext Link aufrufen

DOI / URN:	10.3847/1538-4357/ab61f1

Katalog-ID:	1690146613

Internformat


LEADER	01000caa a2200265 4500
001	1690146613
003	DE-627
005	20220817232235.0
007	cr uuu---uuuuu
008	200217s2020 xx \|\|\|\|\|o 00\| \|\|eng c
024	7		\|a 10.3847/1538-4357/ab61f1 \|2 doi
035			\|a (DE-627)1690146613
035			\|a (DE-599)KXP1690146613
035			\|a (OCoLC)1341305563
040			\|a DE-627 \|b ger \|c DE-627 \|e rda
041			\|a eng
100	1		\|a Jacyszyn-Dobrzeniecka, Anna M. \|e verfasserin \|0 (DE-588)1204861994 \|0 (DE-627)1690145293 \|4 aut
245	1	0	\|a OGLE-ing the Magellanic System \|b Cepheids in the Bridge \|c Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona
264		1	\|c 2020 January 22
300			\|a 16
336			\|a Text \|b txt \|2 rdacontent
337			\|a Computermedien \|b c \|2 rdamedia
338			\|a Online-Ressource \|b cr \|2 rdacarrier
500			\|a Gesehen am 17.02.2020
520			\|a We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds.
773	0	8	\|i Enthalten in \|t The astrophysical journal \|d London : Institute of Physics Publ., 1995 \|g 889(2020,1) Artikel-Nummer 25, 16 Seiten \|h Online-Ressource \|w (DE-627)269019219 \|w (DE-600)1473835-1 \|w (DE-576)077662733 \|x 1538-4357 \|7 nnns
773	1	8	\|g volume:889 \|g year:2020 \|g pages:25 \|g extent:16
856	4	0	\|u https://doi.org/10.3847/1538-4357/ab61f1 \|x Verlag \|x Resolving-System \|3 Volltext
856	4	0	\|u http://adsabs.harvard.edu/abs/2020ApJ...889...25J \|x Verlag
912			\|a GBV_USEFLAG_U
912			\|a GBV_ILN_2013
912			\|a ISIL_DE-16-250
912			\|a SYSFLAG_1
912			\|a GBV_KXP
912			\|a GBV_ILN_11
912			\|a GBV_ILN_20
912			\|a GBV_ILN_22
912			\|a GBV_ILN_23
912			\|a GBV_ILN_24
912			\|a GBV_ILN_31
912			\|a GBV_ILN_39
912			\|a GBV_ILN_40
912			\|a GBV_ILN_60
912			\|a GBV_ILN_62
912			\|a GBV_ILN_63
912			\|a GBV_ILN_65
912			\|a GBV_ILN_69
912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_95
912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_151
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_230
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2088
912			\|a GBV_ILN_2190
912			\|a GBV_ILN_2522
912			\|a GBV_ILN_4012
912			\|a GBV_ILN_4037
912			\|a GBV_ILN_4046
912			\|a GBV_ILN_4112
912			\|a GBV_ILN_4125
912			\|a GBV_ILN_4126
912			\|a GBV_ILN_4249
912			\|a GBV_ILN_4305
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4307
912			\|a GBV_ILN_4313
912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
912			\|a GBV_ILN_4335
912			\|a GBV_ILN_4338
912			\|a GBV_ILN_4367
912			\|a GBV_ILN_4700
951			\|a AR
952			\|d 889 \|j 2020 \|h 25 \|g 16 \|y 889(2020,1) Artikel-Nummer 25, 16 Seiten
980			\|2 2013 \|1 01 \|x DE-16-250 \|b 3595997662 \|c 00 \|f --%%-- \|d --%%-- \|e --%%-- \|j --%%-- \|y l01 \|z 17-02-20
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 00 \|s s \|a hd2020
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 01 \|s s \|0 (DE-627)1410508463 \|a wissenschaftlicher Artikel (Zeitschrift)
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 02 \|s s \|a per_15
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 03 \|s s \|a s_16
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 04 \|s p \|0 (DE-627)1690145536 \|a Jacyszyn-Dobrzeniecka, Anna M.
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 04 \|s k \|0 (DE-627)1428632549 \|a SFB 881 The Milky Way Galaxy
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 04 \|s s \|0 (DE-627)1410501914 \|a Verfasser
982			\|2 2013 \|1 01 \|x DE-16-250 \|8 04 \|s s \|a pos_1

Indexfelder

author_variant	a m j d amj amjd
matchkey_str	article:15384357:2020----::genteaeln
oclc_num	1341305563
hierarchy_sort_str	2020 January 22
publishDate	2020
allfields	10.3847/1538-4357/ab61f1 doi (DE-627)1690146613 (DE-599)KXP1690146613 (OCoLC)1341305563 DE-627 ger DE-627 rda eng Jacyszyn-Dobrzeniecka, Anna M. verfasserin (DE-588)1204861994 (DE-627)1690145293 aut OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona 2020 January 22 16 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 17.02.2020 We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 889(2020,1) Artikel-Nummer 25, 16 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:889 year:2020 pages:25 extent:16 https://doi.org/10.3847/1538-4357/ab61f1 Verlag Resolving-System Volltext http://adsabs.harvard.edu/abs/2020ApJ...889...25J Verlag GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 889 2020 25 16 889(2020,1) Artikel-Nummer 25, 16 Seiten 2013 01 DE-16-250 3595997662 00 --%%-- --%%-- --%%-- --%%-- l01 17-02-20 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_15 2013 01 DE-16-250 03 s s_16 2013 01 DE-16-250 04 p (DE-627)1690145536 Jacyszyn-Dobrzeniecka, Anna M. 2013 01 DE-16-250 04 k (DE-627)1428632549 SFB 881 The Milky Way Galaxy 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_1
spelling	10.3847/1538-4357/ab61f1 doi (DE-627)1690146613 (DE-599)KXP1690146613 (OCoLC)1341305563 DE-627 ger DE-627 rda eng Jacyszyn-Dobrzeniecka, Anna M. verfasserin (DE-588)1204861994 (DE-627)1690145293 aut OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona 2020 January 22 16 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 17.02.2020 We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 889(2020,1) Artikel-Nummer 25, 16 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:889 year:2020 pages:25 extent:16 https://doi.org/10.3847/1538-4357/ab61f1 Verlag Resolving-System Volltext http://adsabs.harvard.edu/abs/2020ApJ...889...25J Verlag GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 889 2020 25 16 889(2020,1) Artikel-Nummer 25, 16 Seiten 2013 01 DE-16-250 3595997662 00 --%%-- --%%-- --%%-- --%%-- l01 17-02-20 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_15 2013 01 DE-16-250 03 s s_16 2013 01 DE-16-250 04 p (DE-627)1690145536 Jacyszyn-Dobrzeniecka, Anna M. 2013 01 DE-16-250 04 k (DE-627)1428632549 SFB 881 The Milky Way Galaxy 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_1
allfields_unstemmed	10.3847/1538-4357/ab61f1 doi (DE-627)1690146613 (DE-599)KXP1690146613 (OCoLC)1341305563 DE-627 ger DE-627 rda eng Jacyszyn-Dobrzeniecka, Anna M. verfasserin (DE-588)1204861994 (DE-627)1690145293 aut OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona 2020 January 22 16 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 17.02.2020 We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 889(2020,1) Artikel-Nummer 25, 16 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:889 year:2020 pages:25 extent:16 https://doi.org/10.3847/1538-4357/ab61f1 Verlag Resolving-System Volltext http://adsabs.harvard.edu/abs/2020ApJ...889...25J Verlag GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 889 2020 25 16 889(2020,1) Artikel-Nummer 25, 16 Seiten 2013 01 DE-16-250 3595997662 00 --%%-- --%%-- --%%-- --%%-- l01 17-02-20 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_15 2013 01 DE-16-250 03 s s_16 2013 01 DE-16-250 04 p (DE-627)1690145536 Jacyszyn-Dobrzeniecka, Anna M. 2013 01 DE-16-250 04 k (DE-627)1428632549 SFB 881 The Milky Way Galaxy 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_1
allfieldsGer	10.3847/1538-4357/ab61f1 doi (DE-627)1690146613 (DE-599)KXP1690146613 (OCoLC)1341305563 DE-627 ger DE-627 rda eng Jacyszyn-Dobrzeniecka, Anna M. verfasserin (DE-588)1204861994 (DE-627)1690145293 aut OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona 2020 January 22 16 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 17.02.2020 We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 889(2020,1) Artikel-Nummer 25, 16 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:889 year:2020 pages:25 extent:16 https://doi.org/10.3847/1538-4357/ab61f1 Verlag Resolving-System Volltext http://adsabs.harvard.edu/abs/2020ApJ...889...25J Verlag GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 889 2020 25 16 889(2020,1) Artikel-Nummer 25, 16 Seiten 2013 01 DE-16-250 3595997662 00 --%%-- --%%-- --%%-- --%%-- l01 17-02-20 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_15 2013 01 DE-16-250 03 s s_16 2013 01 DE-16-250 04 p (DE-627)1690145536 Jacyszyn-Dobrzeniecka, Anna M. 2013 01 DE-16-250 04 k (DE-627)1428632549 SFB 881 The Milky Way Galaxy 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_1
allfieldsSound	10.3847/1538-4357/ab61f1 doi (DE-627)1690146613 (DE-599)KXP1690146613 (OCoLC)1341305563 DE-627 ger DE-627 rda eng Jacyszyn-Dobrzeniecka, Anna M. verfasserin (DE-588)1204861994 (DE-627)1690145293 aut OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona 2020 January 22 16 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 17.02.2020 We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 889(2020,1) Artikel-Nummer 25, 16 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:889 year:2020 pages:25 extent:16 https://doi.org/10.3847/1538-4357/ab61f1 Verlag Resolving-System Volltext http://adsabs.harvard.edu/abs/2020ApJ...889...25J Verlag GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 889 2020 25 16 889(2020,1) Artikel-Nummer 25, 16 Seiten 2013 01 DE-16-250 3595997662 00 --%%-- --%%-- --%%-- --%%-- l01 17-02-20 2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_15 2013 01 DE-16-250 03 s s_16 2013 01 DE-16-250 04 p (DE-627)1690145536 Jacyszyn-Dobrzeniecka, Anna M. 2013 01 DE-16-250 04 k (DE-627)1428632549 SFB 881 The Milky Way Galaxy 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_1
language	English
source	Enthalten in The astrophysical journal 889(2020,1) Artikel-Nummer 25, 16 Seiten volume:889 year:2020 pages:25 extent:16
sourceStr	Enthalten in The astrophysical journal 889(2020,1) Artikel-Nummer 25, 16 Seiten volume:889 year:2020 pages:25 extent:16
format_phy_str_mv	Article
building	2013:0
institution	findex.gbv.de
selectbib_iln_str_mv	2013@01
sw_local_iln_str_mv	2013:hd2020 DE-16-250:hd2020 2013:wissenschaftlicher Artikel (Zeitschrift) DE-16-250:wissenschaftlicher Artikel (Zeitschrift) 2013:per_15 DE-16-250:per_15 2013:s_16 DE-16-250:s_16 2013:Jacyszyn-Dobrzeniecka, Anna M. DE-16-250:Jacyszyn-Dobrzeniecka, Anna M. 2013:SFB 881 The Milky Way Galaxy DE-16-250:SFB 881 The Milky Way Galaxy 2013:Verfasser DE-16-250:Verfasser 2013:pos_1 DE-16-250:pos_1
isfreeaccess_bool	false
container_title	The astrophysical journal
authorswithroles_txt_mv	Jacyszyn-Dobrzeniecka, Anna M. @@aut@@
publishDateDaySort_date	2020-01-01T00:00:00Z
hierarchy_top_id	269019219
id	1690146613
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">1690146613</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220817232235.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">200217s2020 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3847/1538-4357/ab61f1</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)1690146613</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)KXP1690146613</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1341305563</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Jacyszyn-Dobrzeniecka, Anna M.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1204861994</subfield><subfield code="0">(DE-627)1690145293</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">OGLE-ing the Magellanic System</subfield><subfield code="b">Cepheids in the Bridge</subfield><subfield code="c">Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020 January 22</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">16</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Gesehen am 17.02.2020</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds.</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The astrophysical journal</subfield><subfield code="d">London : Institute of Physics Publ., 1995</subfield><subfield code="g">889(2020,1) Artikel-Nummer 25, 16 Seiten</subfield><subfield code="h">Online-Ressource</subfield><subfield code="w">(DE-627)269019219</subfield><subfield code="w">(DE-600)1473835-1</subfield><subfield code="w">(DE-576)077662733</subfield><subfield code="x">1538-4357</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:889</subfield><subfield code="g">year:2020</subfield><subfield code="g">pages:25</subfield><subfield code="g">extent:16</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.3847/1538-4357/ab61f1</subfield><subfield code="x">Verlag</subfield><subfield code="x">Resolving-System</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://adsabs.harvard.edu/abs/2020ApJ...889...25J</subfield><subfield code="x">Verlag</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2013</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ISIL_DE-16-250</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_1</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_KXP</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_65</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_151</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_230</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_702</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2088</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2190</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2522</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4037</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4125</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4249</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4313</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4322</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4323</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4324</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4325</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4335</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4338</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4367</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">889</subfield><subfield code="j">2020</subfield><subfield code="h">25</subfield><subfield code="g">16</subfield><subfield code="y">889(2020,1) Artikel-Nummer 25, 16 Seiten</subfield></datafield><datafield tag="980" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="b">3595997662</subfield><subfield code="c">00</subfield><subfield code="f">--%%--</subfield><subfield code="d">--%%--</subfield><subfield code="e">--%%--</subfield><subfield code="j">--%%--</subfield><subfield code="y">l01</subfield><subfield code="z">17-02-20</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">00</subfield><subfield code="s">s</subfield><subfield code="a">hd2020</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">01</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410508463</subfield><subfield code="a">wissenschaftlicher Artikel (Zeitschrift)</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">02</subfield><subfield code="s">s</subfield><subfield code="a">per_15</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">03</subfield><subfield code="s">s</subfield><subfield code="a">s_16</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">p</subfield><subfield code="0">(DE-627)1690145536</subfield><subfield code="a">Jacyszyn-Dobrzeniecka, Anna M.</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1428632549</subfield><subfield code="a">SFB 881 The Milky Way Galaxy</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410501914</subfield><subfield code="a">Verfasser</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="a">pos_1</subfield></datafield></record></collection>
standort_str_mv	--%%--
standort_iln_str_mv	2013:--%%-- DE-16-250:--%%--
author	Jacyszyn-Dobrzeniecka, Anna M.
spellingShingle	Jacyszyn-Dobrzeniecka, Anna M. 2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_15 2013 s_16 2013 Jacyszyn-Dobrzeniecka, Anna M. 2013 SFB 881 The Milky Way Galaxy 2013 Verfasser 2013 pos_1 OGLE-ing the Magellanic System Cepheids in the Bridge
authorStr	Jacyszyn-Dobrzeniecka, Anna M.
ppnlink_with_tag_str_mv	@@773@@(DE-627)269019219
format	electronic Article
delete_txt_mv	keep
author_role	aut
typewithnormlink_str_mv	Person@(DE-588)1204861994 DifferentiatedPerson@(DE-588)1204861994
collection	KXP SWB GVK
remote_str	true
last_changed_iln_str_mv	2013@17-02-20
illustrated	Not Illustrated
issn	1538-4357
topic_title	2013 01 DE-16-250 00 s hd2020 2013 01 DE-16-250 01 s (DE-627)1410508463 wissenschaftlicher Artikel (Zeitschrift) 2013 01 DE-16-250 02 s per_15 2013 01 DE-16-250 03 s s_16 2013 01 DE-16-250 04 p (DE-627)1690145536 Jacyszyn-Dobrzeniecka, Anna M. 2013 01 DE-16-250 04 k (DE-627)1428632549 SFB 881 The Milky Way Galaxy 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_1 OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona
topic	2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_15 2013 s_16 2013 Jacyszyn-Dobrzeniecka, Anna M. 2013 SFB 881 The Milky Way Galaxy 2013 Verfasser 2013 pos_1
topic_unstemmed	2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_15 2013 s_16 2013 Jacyszyn-Dobrzeniecka, Anna M. 2013 SFB 881 The Milky Way Galaxy 2013 Verfasser 2013 pos_1
topic_browse	2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_15 2013 s_16 2013 Jacyszyn-Dobrzeniecka, Anna M. 2013 SFB 881 The Milky Way Galaxy 2013 Verfasser 2013 pos_1
format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
standort_txtP_mv	--%%--
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	cr
hierarchy_parent_title	The astrophysical journal
normlinkwithtype_str_mv	(DE-588)1204861994@Person (DE-588)1204861994@DifferentiatedPerson
hierarchy_parent_id	269019219
signature	--%%--
signature_str_mv	--%%--
hierarchy_top_title	The astrophysical journal
isfreeaccess_txt	false
familylinks_str_mv	(DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733
normlinkwithrole_str_mv	(DE-588)1204861994@@aut@@
title	OGLE-ing the Magellanic System Cepheids in the Bridge
ctrlnum	(DE-627)1690146613 (DE-599)KXP1690146613 (OCoLC)1341305563
title_full	OGLE-ing the Magellanic System Cepheids in the Bridge Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona
author_sort	Jacyszyn-Dobrzeniecka, Anna M.
journal	The astrophysical journal
journalStr	The astrophysical journal
callnumber-first-code	-
lang_code	eng
isOA_bool	false
recordtype	marc
publishDateSort	2020
contenttype_str_mv	txt
container_start_page	25
author_browse	Jacyszyn-Dobrzeniecka, Anna M.
selectkey	2013:l
container_volume	889
physical	16
format_se	Elektronische Aufsätze
author-letter	Jacyszyn-Dobrzeniecka, Anna M.
title_sub	Cepheids in the Bridge
doi_str_mv	10.3847/1538-4357/ab61f1
normlink	1204861994 1690145293 1410508463 1690145536 1428632549 1410501914
normlink_prefix_str_mv	(DE-588)1204861994 (DE-627)1690145293 (DE-627)1410508463 (DE-627)1690145536 (DE-627)1428632549 (DE-627)1410501914
title_sort	ogle-ing the magellanic systemcepheids in the bridge
title_auth	OGLE-ing the Magellanic System Cepheids in the Bridge
abstract	We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Gesehen am 17.02.2020
abstractGer	We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Gesehen am 17.02.2020
abstract_unstemmed	We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds. Gesehen am 17.02.2020
collection_details	GBV_USEFLAG_U GBV_ILN_2013 ISIL_DE-16-250 SYSFLAG_1 GBV_KXP GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2190 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700
title_short	OGLE-ing the Magellanic System
url	https://doi.org/10.3847/1538-4357/ab61f1 http://adsabs.harvard.edu/abs/2020ApJ...889...25J
ausleihindikator_str_mv	2013:-
rolewithnormlink_str_mv	@@aut@@(DE-588)1204861994
remote_bool	true
ppnlink	269019219
GND_str_mv	Jacyszyn-Dobrzeniecka, Anna Marta Jacyszyn, Anna M. Dobrzeniecka, Anna Jacyszyn- Jacyszyn-Dobrzeniecka, Anna M.
GND_txt_mv	Jacyszyn-Dobrzeniecka, Anna Marta Jacyszyn, Anna M. Dobrzeniecka, Anna Jacyszyn- Jacyszyn-Dobrzeniecka, Anna M.
GND_txtF_mv	Jacyszyn-Dobrzeniecka, Anna Marta Jacyszyn, Anna M. Dobrzeniecka, Anna Jacyszyn- Jacyszyn-Dobrzeniecka, Anna M.
mediatype_str_mv	c
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.3847/1538-4357/ab61f1
callnumber-a	--%%--
up_date	2024-07-04T21:44:42.875Z
_version_	1803686492637233152
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">1690146613</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220817232235.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">200217s2020 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3847/1538-4357/ab61f1</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)1690146613</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)KXP1690146613</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1341305563</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Jacyszyn-Dobrzeniecka, Anna M.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(DE-588)1204861994</subfield><subfield code="0">(DE-627)1690145293</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">OGLE-ing the Magellanic System</subfield><subfield code="b">Cepheids in the Bridge</subfield><subfield code="c">Anna M. Jacyszyn-Dobrzeniecka, Igor Soszyński, Andrzej Udalski, Michał K. Szymański, Dorota M. Skowron, Jan Skowron, Przemek Mróz, Katarzyna Kruszyńska, Patryk Iwanek, Paweł Pietrukowicz, Radosław Poleski, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof Rybicki, and Marcin Wrona</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020 January 22</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">16</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Gesehen am 17.02.2020</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment - Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimensional maps. Classical Cepheid (CC) on-sky locations match very well neutral hydrogen and young stars distributions; thus, they add to the overall young Bridge population. In three dimensions, 8 out of 10 CCs form a bridge-like connection between the Magellanic Clouds. The other two are located slightly farther away and may constitute the Counter Bridge. We estimate ages of our Cepheids to be less than 300 Myr for from 5 up to 8 out of 10, depending on whether the rotation is included. This is in agreement with a scenario where these stars were formed in situ after the last encounter of the Magellanic Clouds. Cepheids' proper motions reveal that they are moving away from both Large and Small Magellanic Clouds. Anomalous Cepheids are more spread than CCs in both two and three dimensions, even though they form a rather smooth connection between the Magellanic Clouds. However, this connection does not seem to be bridge-like, as there are many outliers around both Magellanic Clouds.</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The astrophysical journal</subfield><subfield code="d">London : Institute of Physics Publ., 1995</subfield><subfield code="g">889(2020,1) Artikel-Nummer 25, 16 Seiten</subfield><subfield code="h">Online-Ressource</subfield><subfield code="w">(DE-627)269019219</subfield><subfield code="w">(DE-600)1473835-1</subfield><subfield code="w">(DE-576)077662733</subfield><subfield code="x">1538-4357</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:889</subfield><subfield code="g">year:2020</subfield><subfield code="g">pages:25</subfield><subfield code="g">extent:16</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.3847/1538-4357/ab61f1</subfield><subfield code="x">Verlag</subfield><subfield code="x">Resolving-System</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://adsabs.harvard.edu/abs/2020ApJ...889...25J</subfield><subfield code="x">Verlag</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2013</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ISIL_DE-16-250</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_1</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_KXP</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_23</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_39</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_60</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_65</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_69</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_73</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_95</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_110</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_151</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_161</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_230</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_285</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_293</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_370</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_602</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_702</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2088</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2190</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2522</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4037</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4112</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4125</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4249</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4305</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4313</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4322</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4323</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4324</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4325</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4335</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4338</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4367</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">889</subfield><subfield code="j">2020</subfield><subfield code="h">25</subfield><subfield code="g">16</subfield><subfield code="y">889(2020,1) Artikel-Nummer 25, 16 Seiten</subfield></datafield><datafield tag="980" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="b">3595997662</subfield><subfield code="c">00</subfield><subfield code="f">--%%--</subfield><subfield code="d">--%%--</subfield><subfield code="e">--%%--</subfield><subfield code="j">--%%--</subfield><subfield code="y">l01</subfield><subfield code="z">17-02-20</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">00</subfield><subfield code="s">s</subfield><subfield code="a">hd2020</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">01</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410508463</subfield><subfield code="a">wissenschaftlicher Artikel (Zeitschrift)</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">02</subfield><subfield code="s">s</subfield><subfield code="a">per_15</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">03</subfield><subfield code="s">s</subfield><subfield code="a">s_16</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">p</subfield><subfield code="0">(DE-627)1690145536</subfield><subfield code="a">Jacyszyn-Dobrzeniecka, Anna M.</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">k</subfield><subfield code="0">(DE-627)1428632549</subfield><subfield code="a">SFB 881 The Milky Way Galaxy</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="0">(DE-627)1410501914</subfield><subfield code="a">Verfasser</subfield></datafield><datafield tag="982" ind1=" " ind2=" "><subfield code="2">2013</subfield><subfield code="1">01</subfield><subfield code="x">DE-16-250</subfield><subfield code="8">04</subfield><subfield code="s">s</subfield><subfield code="a">pos_1</subfield></datafield></record></collection>
score	7.3995953

Nicht das Richtige dabei?

Schreiben Sie uns!

OGLE-ing the Magellanic System : Cepheids in the Bridge

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?