Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II

New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Kyu-Dong Oh [verfasserIn] Chun-Hwey Kim [verfasserIn] Ho-iL Kim [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2005

Schlagwörter:	contact binary small mass ratio contact binary binary solution

Übergeordnetes Werk:	In: Journal of Astronomy and Space Sciences - Korean Space Science Society (KSSS), 2012, 22(2005), 3, Seite 223-232
Übergeordnetes Werk:	volume:22 ; year:2005 ; number:3 ; pages:223-232

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.5140/JASS.2005.22.3.223

Katalog-ID:	DOAJ005769620

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spelling	10.5140/JASS.2005.22.3.223 doi (DE-627)DOAJ005769620 (DE-599)DOAJ974db86adf69433f85c1147472e0bcf2 DE-627 ger DE-627 rakwb eng QB1-991 Kyu-Dong Oh verfasserin aut Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II 2005 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD program from the published spectroscopic and newly observed photometric data. The evolutionary status of this type of binary system including V410 Aur and V776 Cas has been considered. We reconfirmed that the primary stars of the low mass contact binary system were located on the TAMS and secondary stars were located under the ZAMS in H-R diagram. contact binary small mass ratio contact binary binary solution Astronomy Chun-Hwey Kim verfasserin aut Ho-iL Kim verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 22(2005), 3, Seite 223-232 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:22 year:2005 number:3 pages:223-232 https://doi.org/10.5140/JASS.2005.22.3.223 kostenfrei https://doaj.org/article/974db86adf69433f85c1147472e0bcf2 kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_223.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 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 22 2005 3 223-232
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allfieldsGer	10.5140/JASS.2005.22.3.223 doi (DE-627)DOAJ005769620 (DE-599)DOAJ974db86adf69433f85c1147472e0bcf2 DE-627 ger DE-627 rakwb eng QB1-991 Kyu-Dong Oh verfasserin aut Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II 2005 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD program from the published spectroscopic and newly observed photometric data. The evolutionary status of this type of binary system including V410 Aur and V776 Cas has been considered. We reconfirmed that the primary stars of the low mass contact binary system were located on the TAMS and secondary stars were located under the ZAMS in H-R diagram. contact binary small mass ratio contact binary binary solution Astronomy Chun-Hwey Kim verfasserin aut Ho-iL Kim verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 22(2005), 3, Seite 223-232 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:22 year:2005 number:3 pages:223-232 https://doi.org/10.5140/JASS.2005.22.3.223 kostenfrei https://doaj.org/article/974db86adf69433f85c1147472e0bcf2 kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_223.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 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 22 2005 3 223-232
allfieldsSound	10.5140/JASS.2005.22.3.223 doi (DE-627)DOAJ005769620 (DE-599)DOAJ974db86adf69433f85c1147472e0bcf2 DE-627 ger DE-627 rakwb eng QB1-991 Kyu-Dong Oh verfasserin aut Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II 2005 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD program from the published spectroscopic and newly observed photometric data. The evolutionary status of this type of binary system including V410 Aur and V776 Cas has been considered. We reconfirmed that the primary stars of the low mass contact binary system were located on the TAMS and secondary stars were located under the ZAMS in H-R diagram. contact binary small mass ratio contact binary binary solution Astronomy Chun-Hwey Kim verfasserin aut Ho-iL Kim verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 22(2005), 3, Seite 223-232 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:22 year:2005 number:3 pages:223-232 https://doi.org/10.5140/JASS.2005.22.3.223 kostenfrei https://doaj.org/article/974db86adf69433f85c1147472e0bcf2 kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_223.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 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 22 2005 3 223-232
language	English
source	In Journal of Astronomy and Space Sciences 22(2005), 3, Seite 223-232 volume:22 year:2005 number:3 pages:223-232
sourceStr	In Journal of Astronomy and Space Sciences 22(2005), 3, Seite 223-232 volume:22 year:2005 number:3 pages:223-232
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	contact binary small mass ratio contact binary binary solution Astronomy
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container_title	Journal of Astronomy and Space Sciences
authorswithroles_txt_mv	Kyu-Dong Oh @@aut@@ Chun-Hwey Kim @@aut@@ Ho-iL Kim @@aut@@
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callnumber-first	Q - Science
author	Kyu-Dong Oh
spellingShingle	Kyu-Dong Oh misc QB1-991 misc contact binary misc small mass ratio contact binary misc binary solution misc Astronomy Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II
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topic_title	QB1-991 Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II contact binary small mass ratio contact binary binary solution
topic	misc QB1-991 misc contact binary misc small mass ratio contact binary misc binary solution misc Astronomy
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title	Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II
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title_full	Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II
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title_sort	low mass ratio contact binary v410 aur and v776 cas - ii
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title_auth	Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II
abstract	New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD program from the published spectroscopic and newly observed photometric data. The evolutionary status of this type of binary system including V410 Aur and V776 Cas has been considered. We reconfirmed that the primary stars of the low mass contact binary system were located on the TAMS and secondary stars were located under the ZAMS in H-R diagram.
abstractGer	New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD program from the published spectroscopic and newly observed photometric data. The evolutionary status of this type of binary system including V410 Aur and V776 Cas has been considered. We reconfirmed that the primary stars of the low mass contact binary system were located on the TAMS and secondary stars were located under the ZAMS in H-R diagram.
abstract_unstemmed	New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory. The absolute dimensions of the low mass ratio contact binaries, V410 Aur and V776 Cas, were obtained using WD program from the published spectroscopic and newly observed photometric data. The evolutionary status of this type of binary system including V410 Aur and V776 Cas has been considered. We reconfirmed that the primary stars of the low mass contact binary system were located on the TAMS and secondary stars were located under the ZAMS in H-R diagram.
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title_short	Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II
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