Thermal instability analysis of the growth of molecular clouds in our Galaxy

Details Thermal instability analysis of the growth of molecular clouds in our Galaxy Thermal instability analysis of the growth of molecular clouds in our Galaxy

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.176...85g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 176, no. 1, Feb. 1991, p. 85-96.

Astronomy and Astrophysics

Astrophysics

1

Milky Way Galaxy, Molecular Clouds, Thermal Stability, Bremsstrahlung, Gravitational Effects, Heat Transfer, Magnetohydrodynamics, Perturbation Theory

Scientific paper

Thermal instability in a high-temperature rotating and gravitating plasma in the central region of our Galaxy has been analyzed in the absence of a magnetic field. The minimum scales of perturbation are calculated using different forms of heat loss function and different values of the parameters involved. The growth rates, the growth times, for these scales are also computed and they have been discussed

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