High Resolution Simulations of Supersonic Turbulence in Molecular Clouds

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dc.creatorKritsuk, Alexei G.
dc.creatorWagner, Rick
dc.creatorNorman, Michael L.
dc.creatorPadoan, Paolo
dc.date2006-07-28
dc.date.accessioned2026-07-07T11:25:50Z
dc.date.available2026-07-07T11:25:50Z
dc.descriptionWe present the results of three-dimensional simulations of supersonic Euler turbulence with grid resolutions up to 1024^3 points. Our numerical experiments describe nonmagnetized driven turbulent flows with an isothermal equation of state and an rms Mach number of 6. We demonstrate that the inertial range scaling properties of turbulence in this strongly compressible regime deviate substantially from a Kolmogorov-like behavior previously recovered for mildly compressible transonic flows.
dc.description7 pages, 8 figures, to appear in ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0607634
dc.identifierhttp://arxiv.org/abs/astro-ph/0607634
dc.identifierASPConf.Ser.359:84-90,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195634
dc.subjectAstrophysics
dc.titleHigh Resolution Simulations of Supersonic Turbulence in Molecular Clouds
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