The Role of Heat-Loss Function on the Growth of Molecular Clouds in our Galaxy

Author:
R.K. PENSIA, ASHOK KUMAR PATIDAR*, VISHAL KUMAR and VIKAS PRAJAPAT
Affiliation:

Post Graduate Department of Physics Govt P.G. College Neemach MP India

Email:-ashok_patidar341@yahoo.co.in

Keyword:
Arbitrary radiative heat-loss function, Suspended Particles, magneto hydrodynamics (MHD). Jeans criterion.
Issue Date:
April 2011
Abstract:

The role of heat-loss function on the growth of molecular clouds in infinite homogenous thermally conducting viscous plasma incorporating permeability in the presence of suspended particles has been investigated. A general dispersion relation is obtained by using the normal mode analysis with the help of relevant linearized perturbation equations of the problem and a modified Jeans criterion of instability is obtained.

Pages:
ISSN:
2319-8052 (Online) - 2231-3478 (Print)
Source:
DOI:
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Copy the following to cite this article:

R.K. PENSIA, ASHOK KUMAR PATIDAR*, VISHAL KUMAR and VIKAS PRAJAPAT, "The Role of Heat-Loss Function on the Growth of Molecular Clouds in our Galaxy ", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 1, Page Number , 2016

Copy the following to cite this URL:

R.K. PENSIA, ASHOK KUMAR PATIDAR*, VISHAL KUMAR and VIKAS PRAJAPAT, "The Role of Heat-Loss Function on the Growth of Molecular Clouds in our Galaxy ", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 1, Page Number , 2016

Available from: http://www.ultraphysicalsciences.org/paper/571/

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