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The development of modes of thermal instability in a non-stationary medium (production of OH maser condensations)

Published online by Cambridge University Press:  03 August 2017

V. V. Burdyuzha
V. V. Burdyuzha*
Affiliation:
Astro-Space Centre Lebedev's Physical, Institute Academy of Sciences or the USSR Profsoyuznaya, 84/32, 117810, Moscow USSR

Abstract

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In a nonstationary medium (behind the shock front, for instance) the development of isobaric and adiabatic modes of the thermal instability are more preferable. Some examples of the fragmentation of the medium on clouds in case of OH masers are given.

Type
Shocks and Instabilities
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 211 - 214
Copyright
Copyright © Kluwer 1991 

References

Burdyuzha, V. V., Ruzmaikina, T. V. 1974, Soviet. Astron. 18, 201.Google Scholar
Burdyuzha, V. V., Ruzmaikina, T. V. 1975, Astron. Astrophys. 40, 233.Google Scholar
Hunter, J. H. 1970, Astrophys. J. 161, 451.Google Scholar
Oppenheimer, M. 1977, Astrophys. J., 211, 400.Google Scholar
Reid, M. J. The Paper at the Thirg Haystack conference, 1990.Google Scholar
Schekinov, Yu. A. 1979, Astrophysica, 15, 347.Google Scholar
Shull, J.H., Hollenbach, D.J. 1978, Astrophys. J., 220, 525.Google Scholar