Cloud dispersal in turbulent flows
dc.contributor.author | Heitsch, Fabian | en_US |
dc.contributor.author | Slyz, A. D. | en_US |
dc.contributor.author | Devriendt, J. E. G. | en_US |
dc.contributor.author | Burkert, Andreas | en_US |
dc.date.accessioned | 2010-06-01T19:18:22Z | |
dc.date.available | 2010-06-01T19:18:22Z | |
dc.date.issued | 2006-12-21 | en_US |
dc.identifier.citation | Heitsch, F.; Slyz, A. D.; Devriendt, J. E. G.; Burkert, A. (2006). "Cloud dispersal in turbulent flows." Monthly Notices of the Royal Astronomical Society 373(4): 1379-1388. <http://hdl.handle.net/2027.42/72450> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/72450 | |
dc.description.abstract | Cold clouds embedded in warm media are very common objects in astrophysics. Their disruption time-scale depends strongly on the dynamical configuration. We discuss the evolution of an initially homogeneous cold cloud embedded in warm turbulent gas. Within a couple of dynamical time-scales, the filling factor of the cold gas within the original cloud radius drops below 50 per cent. Turbulent diffusivities estimated from the time evolution of radial filling factor profiles are not constant with time. Cold and warm gas are bodily transported by turbulence and mixed. This is only mildly indicated by column density maps. The radiation field within the cloud, however, increases by several orders of magnitudes due to the mixing, with possible consequences for cloud chemistry and evolution within a few dynamical time-scales. | en_US |
dc.format.extent | 2878029 bytes | |
dc.format.extent | 3109 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.publisher | Blackwell Publishing Ltd | en_US |
dc.rights | 2006 The Authors. Journal compilation © 2006 RAS | en_US |
dc.subject.other | Hydrodynamics | en_US |
dc.subject.other | Radiative Transfer | en_US |
dc.subject.other | Turbulence | en_US |
dc.subject.other | ISM: Clouds | en_US |
dc.subject.other | ISM: Kinematics and Dynamics | en_US |
dc.title | Cloud dispersal in turbulent flows | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USA | en_US |
dc.contributor.affiliationother | University Observatory Munich, Scheinerstr. 1, 81679 Munich, Germany | en_US |
dc.contributor.affiliationother | UniversitÉ de Lyon 1, Centre de Recherche Astronomique de Lyon, Observatoire de Lyon, 9 Avenue Charles AndrÉ, F-69230 Saint-Genis Laval, France; CNRS, UMR 5574, Ecole Normale SupÉrieure de Lyon | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/72450/1/j.1365-2966.2006.11164.x.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2006.11164.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
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