A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms
We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various p...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Pineda Gálvez, Jorge Luis - 1979- [verfasserIn] Stutzki, Jürgen - 1956- [verfasserIn] Buchbender, Christof [verfasserIn] Koda, Jin [verfasserIn] Fischer, Christian [verfasserIn] Goldsmith, Paul F. - 1948- [verfasserIn] Glover, Simon [verfasserIn] Klessen, Ralf S. - 1968- [verfasserIn] Kramer, Carsten Sven - 1983- [verfasserIn] Mookerjea, Bhaswati [verfasserIn] Smith, Rowan J. - 1984- [verfasserIn] Treß, Robin G. - 1987- [verfasserIn] Ziebart, Monika [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020 September 9 |
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| Anmerkung: |
Gesehen am 22.10.2020 |
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| Umfang: |
17 |
| Übergeordnetes Werk: |
Enthalten in: The astrophysical journal - London : Institute of Physics Publ., 1995, 900(2020) Artikel-Nummer 132, 17 Seiten |
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| Übergeordnetes Werk: |
volume:900 ; year:2020 ; extent:17 |
| Links: |
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| DOI / URN: |
10.3847/1538-4357/abab0a |
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| Katalog-ID: |
1736236318 |
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| 245 | 1 | 2 | |a A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms |c Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart |
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| 520 | |a We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. | ||
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| 700 | 1 | |a Buchbender, Christof |e verfasserin |4 aut | |
| 700 | 1 | |a Koda, Jin |e verfasserin |4 aut | |
| 700 | 1 | |a Fischer, Christian |e verfasserin |4 aut | |
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| 700 | 1 | |a Ziebart, Monika |e verfasserin |4 aut | |
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10.3847/1538-4357/abab0a doi (DE-627)1736236318 (DE-599)KXP1736236318 (OCoLC)1341373123 DE-627 ger DE-627 rda eng Pineda Gálvez, Jorge Luis 1979- verfasserin (DE-588)133333469 (DE-627)543372839 (DE-576)299778487 aut A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart C II second 2020 September 9 17 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 22.10.2020 We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Stutzki, Jürgen 1956- verfasserin (DE-588)1152015176 (DE-627)101322826X (DE-576)163238383 aut Buchbender, Christof verfasserin aut Koda, Jin verfasserin aut Fischer, Christian verfasserin aut Goldsmith, Paul F. 1948- verfasserin (DE-588)135735637 (DE-627)693735600 (DE-576)300617321 aut Glover, Simon verfasserin (DE-588)1043520449 (DE-627)770635903 (DE-576)394879252 aut Klessen, Ralf S. 1968- verfasserin (DE-588)120533820 (DE-627)392381532 (DE-576)178685399 aut Kramer, Carsten Sven 1983- verfasserin (DE-588)105032367X (DE-627)783852673 (DE-576)404525229 aut Mookerjea, Bhaswati verfasserin aut Smith, Rowan J. 1984- verfasserin (DE-588)105834367X (DE-627)796712972 (DE-576)414348001 aut Treß, Robin G. 1987- verfasserin (DE-588)1137196254 (DE-627)894165542 (DE-576)491144814 aut Ziebart, Monika verfasserin aut Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 900(2020) Artikel-Nummer 132, 17 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:900 year:2020 extent:17 https://doi.org/10.3847/1538-4357/abab0a Verlag Resolving-System lizenzpflichtig Volltext 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 900 2020 17 900(2020) Artikel-Nummer 132, 17 Seiten 2013 01 DE-16-250 3784416373 00 --%%-- --%%-- --%%-- --%%-- l01 22-10-20 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_13 2013 01 DE-16-250 03 s s_17 2013 01 DE-16-250 04 p (DE-627)1464887047 Glover, Simon 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_7 2013 01 DE-16-250 05 p (DE-627)1445553155 Klessen, Ralf S. 2013 01 DE-16-250 05 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 05 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_8 2013 01 DE-16-250 06 p (DE-627)172696907X Kramer, Carsten Sven 2013 01 DE-16-250 06 k (DE-627)1416534733 Fakultät für Chemie und Geowissenschaften 2013 01 DE-16-250 06 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 06 s pos_9 2013 01 DE-16-250 07 p (DE-627)1561145386 Treß, Robin G. 2013 01 DE-16-250 07 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 07 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 07 s pos_12 |
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10.3847/1538-4357/abab0a doi (DE-627)1736236318 (DE-599)KXP1736236318 (OCoLC)1341373123 DE-627 ger DE-627 rda eng Pineda Gálvez, Jorge Luis 1979- verfasserin (DE-588)133333469 (DE-627)543372839 (DE-576)299778487 aut A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart C II second 2020 September 9 17 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 22.10.2020 We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Stutzki, Jürgen 1956- verfasserin (DE-588)1152015176 (DE-627)101322826X (DE-576)163238383 aut Buchbender, Christof verfasserin aut Koda, Jin verfasserin aut Fischer, Christian verfasserin aut Goldsmith, Paul F. 1948- verfasserin (DE-588)135735637 (DE-627)693735600 (DE-576)300617321 aut Glover, Simon verfasserin (DE-588)1043520449 (DE-627)770635903 (DE-576)394879252 aut Klessen, Ralf S. 1968- verfasserin (DE-588)120533820 (DE-627)392381532 (DE-576)178685399 aut Kramer, Carsten Sven 1983- verfasserin (DE-588)105032367X (DE-627)783852673 (DE-576)404525229 aut Mookerjea, Bhaswati verfasserin aut Smith, Rowan J. 1984- verfasserin (DE-588)105834367X (DE-627)796712972 (DE-576)414348001 aut Treß, Robin G. 1987- verfasserin (DE-588)1137196254 (DE-627)894165542 (DE-576)491144814 aut Ziebart, Monika verfasserin aut Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 900(2020) Artikel-Nummer 132, 17 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:900 year:2020 extent:17 https://doi.org/10.3847/1538-4357/abab0a Verlag Resolving-System lizenzpflichtig Volltext 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 900 2020 17 900(2020) Artikel-Nummer 132, 17 Seiten 2013 01 DE-16-250 3784416373 00 --%%-- --%%-- --%%-- --%%-- l01 22-10-20 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_13 2013 01 DE-16-250 03 s s_17 2013 01 DE-16-250 04 p (DE-627)1464887047 Glover, Simon 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_7 2013 01 DE-16-250 05 p (DE-627)1445553155 Klessen, Ralf S. 2013 01 DE-16-250 05 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 05 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_8 2013 01 DE-16-250 06 p (DE-627)172696907X Kramer, Carsten Sven 2013 01 DE-16-250 06 k (DE-627)1416534733 Fakultät für Chemie und Geowissenschaften 2013 01 DE-16-250 06 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 06 s pos_9 2013 01 DE-16-250 07 p (DE-627)1561145386 Treß, Robin G. 2013 01 DE-16-250 07 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 07 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 07 s pos_12 |
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10.3847/1538-4357/abab0a doi (DE-627)1736236318 (DE-599)KXP1736236318 (OCoLC)1341373123 DE-627 ger DE-627 rda eng Pineda Gálvez, Jorge Luis 1979- verfasserin (DE-588)133333469 (DE-627)543372839 (DE-576)299778487 aut A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart C II second 2020 September 9 17 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 22.10.2020 We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Stutzki, Jürgen 1956- verfasserin (DE-588)1152015176 (DE-627)101322826X (DE-576)163238383 aut Buchbender, Christof verfasserin aut Koda, Jin verfasserin aut Fischer, Christian verfasserin aut Goldsmith, Paul F. 1948- verfasserin (DE-588)135735637 (DE-627)693735600 (DE-576)300617321 aut Glover, Simon verfasserin (DE-588)1043520449 (DE-627)770635903 (DE-576)394879252 aut Klessen, Ralf S. 1968- verfasserin (DE-588)120533820 (DE-627)392381532 (DE-576)178685399 aut Kramer, Carsten Sven 1983- verfasserin (DE-588)105032367X (DE-627)783852673 (DE-576)404525229 aut Mookerjea, Bhaswati verfasserin aut Smith, Rowan J. 1984- verfasserin (DE-588)105834367X (DE-627)796712972 (DE-576)414348001 aut Treß, Robin G. 1987- verfasserin (DE-588)1137196254 (DE-627)894165542 (DE-576)491144814 aut Ziebart, Monika verfasserin aut Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 900(2020) Artikel-Nummer 132, 17 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:900 year:2020 extent:17 https://doi.org/10.3847/1538-4357/abab0a Verlag Resolving-System lizenzpflichtig Volltext 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 900 2020 17 900(2020) Artikel-Nummer 132, 17 Seiten 2013 01 DE-16-250 3784416373 00 --%%-- --%%-- --%%-- --%%-- l01 22-10-20 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_13 2013 01 DE-16-250 03 s s_17 2013 01 DE-16-250 04 p (DE-627)1464887047 Glover, Simon 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_7 2013 01 DE-16-250 05 p (DE-627)1445553155 Klessen, Ralf S. 2013 01 DE-16-250 05 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 05 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_8 2013 01 DE-16-250 06 p (DE-627)172696907X Kramer, Carsten Sven 2013 01 DE-16-250 06 k (DE-627)1416534733 Fakultät für Chemie und Geowissenschaften 2013 01 DE-16-250 06 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 06 s pos_9 2013 01 DE-16-250 07 p (DE-627)1561145386 Treß, Robin G. 2013 01 DE-16-250 07 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 07 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 07 s pos_12 |
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10.3847/1538-4357/abab0a doi (DE-627)1736236318 (DE-599)KXP1736236318 (OCoLC)1341373123 DE-627 ger DE-627 rda eng Pineda Gálvez, Jorge Luis 1979- verfasserin (DE-588)133333469 (DE-627)543372839 (DE-576)299778487 aut A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart C II second 2020 September 9 17 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 22.10.2020 We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Stutzki, Jürgen 1956- verfasserin (DE-588)1152015176 (DE-627)101322826X (DE-576)163238383 aut Buchbender, Christof verfasserin aut Koda, Jin verfasserin aut Fischer, Christian verfasserin aut Goldsmith, Paul F. 1948- verfasserin (DE-588)135735637 (DE-627)693735600 (DE-576)300617321 aut Glover, Simon verfasserin (DE-588)1043520449 (DE-627)770635903 (DE-576)394879252 aut Klessen, Ralf S. 1968- verfasserin (DE-588)120533820 (DE-627)392381532 (DE-576)178685399 aut Kramer, Carsten Sven 1983- verfasserin (DE-588)105032367X (DE-627)783852673 (DE-576)404525229 aut Mookerjea, Bhaswati verfasserin aut Smith, Rowan J. 1984- verfasserin (DE-588)105834367X (DE-627)796712972 (DE-576)414348001 aut Treß, Robin G. 1987- verfasserin (DE-588)1137196254 (DE-627)894165542 (DE-576)491144814 aut Ziebart, Monika verfasserin aut Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 900(2020) Artikel-Nummer 132, 17 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:900 year:2020 extent:17 https://doi.org/10.3847/1538-4357/abab0a Verlag Resolving-System lizenzpflichtig Volltext 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 900 2020 17 900(2020) Artikel-Nummer 132, 17 Seiten 2013 01 DE-16-250 3784416373 00 --%%-- --%%-- --%%-- --%%-- l01 22-10-20 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_13 2013 01 DE-16-250 03 s s_17 2013 01 DE-16-250 04 p (DE-627)1464887047 Glover, Simon 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_7 2013 01 DE-16-250 05 p (DE-627)1445553155 Klessen, Ralf S. 2013 01 DE-16-250 05 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 05 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_8 2013 01 DE-16-250 06 p (DE-627)172696907X Kramer, Carsten Sven 2013 01 DE-16-250 06 k (DE-627)1416534733 Fakultät für Chemie und Geowissenschaften 2013 01 DE-16-250 06 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 06 s pos_9 2013 01 DE-16-250 07 p (DE-627)1561145386 Treß, Robin G. 2013 01 DE-16-250 07 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 07 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 07 s pos_12 |
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10.3847/1538-4357/abab0a doi (DE-627)1736236318 (DE-599)KXP1736236318 (OCoLC)1341373123 DE-627 ger DE-627 rda eng Pineda Gálvez, Jorge Luis 1979- verfasserin (DE-588)133333469 (DE-627)543372839 (DE-576)299778487 aut A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart C II second 2020 September 9 17 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Gesehen am 22.10.2020 We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Stutzki, Jürgen 1956- verfasserin (DE-588)1152015176 (DE-627)101322826X (DE-576)163238383 aut Buchbender, Christof verfasserin aut Koda, Jin verfasserin aut Fischer, Christian verfasserin aut Goldsmith, Paul F. 1948- verfasserin (DE-588)135735637 (DE-627)693735600 (DE-576)300617321 aut Glover, Simon verfasserin (DE-588)1043520449 (DE-627)770635903 (DE-576)394879252 aut Klessen, Ralf S. 1968- verfasserin (DE-588)120533820 (DE-627)392381532 (DE-576)178685399 aut Kramer, Carsten Sven 1983- verfasserin (DE-588)105032367X (DE-627)783852673 (DE-576)404525229 aut Mookerjea, Bhaswati verfasserin aut Smith, Rowan J. 1984- verfasserin (DE-588)105834367X (DE-627)796712972 (DE-576)414348001 aut Treß, Robin G. 1987- verfasserin (DE-588)1137196254 (DE-627)894165542 (DE-576)491144814 aut Ziebart, Monika verfasserin aut Enthalten in The astrophysical journal London : Institute of Physics Publ., 1995 900(2020) Artikel-Nummer 132, 17 Seiten Online-Ressource (DE-627)269019219 (DE-600)1473835-1 (DE-576)077662733 1538-4357 nnns volume:900 year:2020 extent:17 https://doi.org/10.3847/1538-4357/abab0a Verlag Resolving-System lizenzpflichtig Volltext 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 900 2020 17 900(2020) Artikel-Nummer 132, 17 Seiten 2013 01 DE-16-250 3784416373 00 --%%-- --%%-- --%%-- --%%-- l01 22-10-20 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_13 2013 01 DE-16-250 03 s s_17 2013 01 DE-16-250 04 p (DE-627)1464887047 Glover, Simon 2013 01 DE-16-250 04 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 04 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 04 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 04 s pos_7 2013 01 DE-16-250 05 p (DE-627)1445553155 Klessen, Ralf S. 2013 01 DE-16-250 05 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 05 k (DE-627)1583940421 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 01 DE-16-250 05 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 05 s pos_8 2013 01 DE-16-250 06 p (DE-627)172696907X Kramer, Carsten Sven 2013 01 DE-16-250 06 k (DE-627)1416534733 Fakultät für Chemie und Geowissenschaften 2013 01 DE-16-250 06 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 06 s pos_9 2013 01 DE-16-250 07 p (DE-627)1561145386 Treß, Robin G. 2013 01 DE-16-250 07 k (DE-627)1416733752 ZAH Institut für Theoretische Astrophysik 2013 01 DE-16-250 07 s (DE-627)1410501914 Verfasser 2013 01 DE-16-250 07 s pos_12 |
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The astrophysical journal |
| authorswithroles_txt_mv |
Pineda Gálvez, Jorge Luis @@aut@@ Stutzki, Jürgen @@aut@@ Buchbender, Christof @@aut@@ Koda, Jin @@aut@@ Fischer, Christian @@aut@@ Goldsmith, Paul F. @@aut@@ Glover, Simon @@aut@@ Klessen, Ralf S. @@aut@@ Kramer, Carsten Sven @@aut@@ Mookerjea, Bhaswati @@aut@@ Smith, Rowan J. @@aut@@ Treß, Robin G. @@aut@@ Ziebart, Monika @@aut@@ |
| publishDateDaySort_date |
2020-01-01T00:00:00Z |
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269019219 |
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1736236318 |
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englisch |
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II. [C II] and CO kinematics across the spiral arms</subfield><subfield code="c">Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. 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[C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. 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Pineda Gálvez, Jorge Luis 1979- |
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Pineda Gálvez, Jorge Luis 1979- 2013 hd2020 2013 wissenschaftlicher Artikel (Zeitschrift) 2013 per_13 2013 s_17 2013 Glover, Simon 2013 ZAH Institut für Theoretische Astrophysik 2013 Exzellenzcluster "STRUKTUREN: Emergenz in Natur, Mathematik und komplexen Daten" 2013 Verfasser 2013 pos_7 2013 Klessen, Ralf S. 2013 pos_8 2013 Kramer, Carsten Sven 2013 Fakultät für Chemie und Geowissenschaften 2013 pos_9 2013 Treß, Robin G. 2013 pos_12 A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms |
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Pineda Gálvez, Jorge Luis 1979- |
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A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms |
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A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms Jorge L. Pineda, Jürgen Stutzki, Christof Buchbender, Jin Koda, Christian Fischer, Paul F. Goldsmith, Simon C.O. Glover, Ralf S. Klessen, Carsten Kramer, Bhaswati Mookerjea, Rowan Smith, Robin Treß and Monika Ziebart |
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sofia survey of [c ii] in the galaxy m51. ii. [c ii] and co kinematics across the spiral arms |
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A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms |
| abstract |
We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Gesehen am 22.10.2020 |
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We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Gesehen am 22.10.2020 |
| abstract_unstemmed |
We present the first complete, velocity-resolved [C ii] 158 μm image of the M51 grand-design spiral galaxy, observed with the upgraded German Receiver for Astronomy at Terahertz frequencies instrument on the Stratospheric Observatory for Infrared Astronomy. [C ii] is an important tracer of various phases of the interstellar medium (ISM), including ionized gas, neutral atomic, and diffuse molecular regions. We combine the [C ii] data with H i, CO, 24 μm dust continuum, FUV, and NIR K-band observations to study the evolution of the ISM across M51's spiral arms in both position-position and position-velocity space. Our data show strong velocity gradients in H i, 12CO, and [C ii] at the locations of the stellar arms (traced by K-band data) with a clear offset in position-velocity space between upstream molecular gas (traced by 12CO) and downstream star formation (traced by [C ii]). We compare the observed position-velocity maps across the spiral arms with synthetic observations from numerical simulations of galaxies with both dynamical and quasi-stationary steady spiral arms that predict both tangential and radial velocities at the location of the spiral arms. We find that our observations, based on the observed velocity gradients and associated offset between CO and [C ii], are consistent with the presence of shocks in the spiral arms in the inner parts of M51 and in the arm connecting the companion galaxy, M51b, in the outer parts of M51. Gesehen am 22.10.2020 |
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A SOFIA survey of [C II] in the galaxy M51. II. [C II] and CO kinematics across the spiral arms |
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