| |  Online-Ressource |
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| Verfasst von: | Soler, Juan D. [VerfasserIn]  |
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| | Beuther, Henrik [VerfasserIn] |
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| | Syed, Jonas [VerfasserIn] |
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| | Wang, Y. [VerfasserIn] |
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| | Henning, Th [VerfasserIn] |
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| | Glover, Simon [VerfasserIn] |
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| | Klessen, Ralf S. [VerfasserIn] |
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| | Sormani, Mattia C. [VerfasserIn] |
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| | Heyer, M. [VerfasserIn] |
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| | Smith, R. J. [VerfasserIn] |
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| | Urquhart, J. S. [VerfasserIn] |
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| | Yang, J. [VerfasserIn] |
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| | Su, Y. [VerfasserIn] |
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| | Zhou, X. [VerfasserIn] |
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| Titel: | The filamentary structures in the CO emission toward the Milky Way disk |
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| Verf.angabe: | J.D. Soler, H. Beuther, J. Syed, Y. Wang, Th. Henning, S.C.O. Glover, R.S. Klessen, M.C. Sormani, M. Heyer, R.J. Smith, J.S. Urquhart, J. Yang, Y. Su, and X. Zhou |
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| Jahr: | 2021 |
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| Umfang: | 8 S. |
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| Fussnoten: | Gesehen am 15.09.2021 |
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| Titel Quelle: | Enthalten in: Astronomy and astrophysics |
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| Ort Quelle: | Les Ulis : EDP Sciences, 1969 |
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| Jahr Quelle: | 2021 |
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| Band/Heft Quelle: | 651(2021), Artikel-ID L4, Seite 1-8 |
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| ISSN Quelle: | 1432-0746 |
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| Abstract: | We present a statistical study of the filamentary structure orientation in the CO emission observations obtained in the Milky Way Imaging Scroll Painting survey in the range 25 (.)degrees . degrees 8 < l < 49 (.)degrees . degrees 7, |b| <= 1 (.)degrees degrees 25, and -100 < v(LSR) < 135 km s(-1). We found that most of the filamentary structures in the (CO)-C-12 and (CO)-C-13 emission do not show a global preferential orientation either parallel or perpendicular to the Galactic plane. However, we found ranges in Galactic longitude and radial velocity where the (CO)-C-12 and (CO)-C-13 filamentary structures are parallel to the Galactic plane. These preferential orientations are different from those found for the HI emission. We consider this an indication that the molecular structures do not simply inherit these properties from parental atomic clouds. Instead, they are shaped by local physical conditions, such as stellar feedback, magnetic fields, and Galactic spiral shocks. |
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| DOI: | doi:10.1051/0004-6361/202141327 |
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| URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.
Volltext: https://doi.org/10.1051/0004-6361/202141327 |
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| | Volltext: https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=DOISource&SrcApp=WOS&KeyAID=10.1051%2F0004-63 ... |
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| | DOI: https://doi.org/10.1051/0004-6361/202141327 |
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| Datenträger: | Online-Ressource |
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| Sprache: | eng |
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| Sach-SW: | clouds |
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| | diffuse |
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| | galaxies: structure |
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| | gradients |
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| | hi/oh/recombination line survey |
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| | ISM: clouds |
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| | ISM: kinematics and dynamics |
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| | ISM: molecules |
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| | ISM: structure |
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| | magnetic-field |
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| | mass |
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| | molecular data |
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| | molecular gas |
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| | orientation |
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| | star-formation |
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| | turbulence |
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| K10plus-PPN: | 1770735283 |
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| Verknüpfungen: | → Zeitschrift |
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¬The¬ filamentary structures in the CO emission toward the Milky Way disk / Soler, Juan D. [VerfasserIn]; 2021 (Online-Ressource)
