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Cloud dispersal in turbulent flows

dc.contributor.authorHeitsch, Fabianen_US
dc.contributor.authorSlyz, A. D.en_US
dc.contributor.authorDevriendt, J. E. G.en_US
dc.contributor.authorBurkert, Andreasen_US
dc.date.accessioned2010-06-01T19:18:22Z
dc.date.available2010-06-01T19:18:22Z
dc.date.issued2006-12-21en_US
dc.identifier.citationHeitsch, 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.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/72450
dc.description.abstractCold 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.extent2878029 bytes
dc.format.extent3109 bytes
dc.format.mimetypeapplication/pdf
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dc.publisherBlackwell Publishing Ltden_US
dc.rights2006 The Authors. Journal compilation © 2006 RASen_US
dc.subject.otherHydrodynamicsen_US
dc.subject.otherRadiative Transferen_US
dc.subject.otherTurbulenceen_US
dc.subject.otherISM: Cloudsen_US
dc.subject.otherISM: Kinematics and Dynamicsen_US
dc.titleCloud dispersal in turbulent flowsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USAen_US
dc.contributor.affiliationotherUniversity Observatory Munich, Scheinerstr. 1, 81679 Munich, Germanyen_US
dc.contributor.affiliationotherUniversitÉ 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 Lyonen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/72450/1/j.1365-2966.2006.11164.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2006.11164.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
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