Supersonic turbulence and structure of interstellar molecular clouds

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dc.creatorBoldyrev, Stanislav
dc.creatorNordlund, Aake
dc.creatorPadoan, Paolo
dc.date2002-03-25
dc.date.accessioned2026-07-07T10:31:13Z
dc.date.available2026-07-07T10:31:13Z
dc.descriptionThe interstellar medium (ISM) provides a unique laboratory for highly supersonic, driven hydrodynamics turbulence. We present a theory of such turbulence, confirm it by numerical simulations, and use the results to explain observational properties of interstellar molecular clouds, the regions where stars are born.
dc.description5 pages, 3 figures included
dc.identifierhttps://arxiv.org/abs/astro-ph/0203452
dc.identifierhttp://arxiv.org/abs/astro-ph/0203452
dc.identifierPhys.Rev.Lett.89:031102,2002
dc.identifierdoi:10.1103/PhysRevLett.89.031102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178337
dc.subjectAstrophysics
dc.subjectChaotic Dynamics
dc.subjectFluid Dynamics
dc.titleSupersonic turbulence and structure of interstellar molecular clouds
dc.typetext

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