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Cloud formation in ...
Cloud formation in the atomic and molecular phase: H I self absorption (HISA) towards a giant molecular filament
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- Wang, Y. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Bihr, S. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Beuther, H. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Rugel, M. R. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Soler, J. D. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Ott, J. (författare)
- National Radio Astronomy Observatory Socorro
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- Kainulainen, Jouni, 1979 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Schneider, N. (författare)
- Universität zu Köln,University of Cologne
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- Klessen, R. S. (författare)
- Ruprecht-Karls-Universität Heidelberg,Heidelberg University
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- Glover, S. C. O. (författare)
- Ruprecht-Karls-Universität Heidelberg,Heidelberg University
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- McClure-Griffiths, N. M. (författare)
- Australian National University
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- Goldsmith, P. F. (författare)
- California Institute of Technology (Caltech)
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- Johnston, K. G. (författare)
- University of Leeds
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- Menten, K. M. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Ragan, S. (författare)
- Cardiff University
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- Anderson, L. D. (författare)
- Green Bank Observatory,West Virginia University
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- Urquhart, J. S. (författare)
- University Of Kent
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- Linz, H. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Roy, N. (författare)
- Indian Institute of Science
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- Smith, R. J. (författare)
- University of Manchester
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Bigiel, F. (författare)
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- Henning, T. (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Longmore, S. N. (författare)
- Liverpool John Moores University
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Max Planck Gesellschaft zur Förderung der Wissenschaften eV. (MPG) National Radio Astronomy Observatory Socorro (creator_code:org_t)
- 2020-02-27
- 2020
- Engelska.
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 634
- Relaterad länk:
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https://research.cha... (primary) (free)
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https://www.aanda.or...
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https://research.cha...
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https://research.cha...
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- Molecular clouds form from the atomic phase of the interstellar medium. However, characterizing the transition between the atomic and the molecular interstellar medium (ISM) is a complex observational task. Here we address cloud formation processes by combining HI self absorption (HISA) with molecular line data. Column density probability density functions (N-PDFs) are a common tool for examining molecular clouds. One scenario proposed by numerical simulations is that the N-PDF evolves from a log-normal shape at early times to a power-law-like shape at later times. To date, investigations of N-PDFs have been mostly limited to the molecular component of the cloud. In this paper, we study the cold atomic component of the giant molecular filament GMF38.1-32.4a (GMF38a, distance = 3.4 kpc, length similar to 230 pc), calculate its N-PDFs, and study its kinematics. We identify an extended HISA feature, which is partly correlated with the (CO)-C-13 emission. The peak velocities of the HISA and (CO)-C-13 observations agree well on the eastern side of the filament, whereas a velocity offset of approximately 4 km s(-1) is found on the western side. The sonic Mach number we derive from the linewidth measurements shows that a large fraction of the HISA, which is ascribed to the cold neutral medium (CNM), is at subsonic and transonic velocities. The column density of the CNM part is on the order of 10(20) to 10(21) cm(-2). The column density of molecular hydrogen, traced by (CO)-C-13, is an order of magnitude higher. The N-PDFs from HISA (CNM), HI emission (the warm and cold neutral medium), and (CO)-C-13 (molecular component) are well described by log-normal functions, which is in agreement with turbulent motions being the main driver of cloud dynamics. The N-PDF of the molecular component also shows a power law in the high column-density region, indicating self-gravity. We suggest that we are witnessing two different evolutionary stages within the filament. The eastern subregion seems to be forming a molecular cloud out of the atomic gas, whereas the western subregion already shows high column density peaks, active star formation, and evidence of related feedback processes.
Ämnesord
- NATURVETENSKAP -- Kemi -- Fysikalisk kemi (hsv//swe)
- NATURAL SCIENCES -- Chemical Sciences -- Physical Chemistry (hsv//eng)
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
- NATURVETENSKAP -- Kemi -- Teoretisk kemi (hsv//swe)
- NATURAL SCIENCES -- Chemical Sciences -- Theoretical Chemistry (hsv//eng)
Nyckelord
- ISM: atoms
- radio lines: ISM
- stars: formation
- ISM: molecules
- ISM: clouds
Publikations- och innehållstyp
- art (ämneskategori)
- ref (ämneskategori)
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Till lärosätets databas
- Av författaren/redakt...
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Wang, Y.
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Bihr, S.
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Beuther, H.
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Rugel, M. R.
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Soler, J. D.
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Ott, J.
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visa fler...
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Kainulainen, Jou ...
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Schneider, N.
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Klessen, R. S.
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Glover, S. C. O.
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McClure-Griffith ...
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Goldsmith, P. F.
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Johnston, K. G.
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Menten, K. M.
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Ragan, S.
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Anderson, L. D.
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Urquhart, J. S.
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Linz, H.
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Roy, N.
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Smith, R. J.
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Bigiel, F.
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Henning, T.
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Longmore, S. N.
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visa färre...
- Om ämnet
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- NATURVETENSKAP
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NATURVETENSKAP
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och Kemi
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och Fysikalisk kemi
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- NATURVETENSKAP
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NATURVETENSKAP
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och Fysik
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och Astronomi astrof ...
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- NATURVETENSKAP
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NATURVETENSKAP
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och Kemi
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och Teoretisk kemi
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Astronomy and As ...
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Chalmers tekniska högskola