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The Density and the Velocity Power Spectrum in Thermally Bi-stable Flows

Published online by Cambridge University Press:  12 August 2011

Adriana Gazol  and
Jongsoo Kim
Adriana Gazol
Affiliation:
Centro de Radioastronomía y Astrofísica UNAM, A. P. 3-72, c.p. 58089, Morelia, Michoacán, México email: a.gazol@crya.unam.mx
Jongsoo Kim
Affiliation:
Korea Astronomy and Space Science Institute, 61-1, Hwaam-Dong, Yuseong-Ku, Daejeon 305-348, Korea email: jskim@kasi.re.kr
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Abstract

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We present numerical results concerning the behavior of the density and the velocity power spectrum in turbulent thermally bistable flows for different Mach numbers.

Keywords

turbulenceinstabilitiesISM: kinematics and dynamicsISM: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S271: Astrophysical Dynamics: From Stars to Galaxies , June 2010 , pp. 379 - 380
Copyright
Copyright © International Astronomical Union 2011

References

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Scalo, J. & Elmegreen, B. G. 2004, ARAA, 42, 275Google Scholar