Thermosolutal-convective instability in a stellar atmosphere

descriptionPublicationkeyboard_double_arrow_right Article 01 Dec 1987 English Publisher:Springer Science and Business Media LLCJournal:Journal of Astrophysics and Astronomy, volume 8, pages 305-314 (issn: 0250-6335, eissn: 0973-7758,

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Authors: R. C. Sharma; Bakshis Singh;

doi: 10.1007/bf02714895

Thermosolutal-convective instability in a stellar atmosphere

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Abstract

The thermosolutal-convective instability of a stellar atomsphere is studied in the presence of suspended particles. The criteria for monotonic instability are derived and are found to hold good also in the presence of uniform rotation and uniform magnetic field on the thermosolutal-convective instability. The thermosolutal-convective instability of a stellar atmosphere is also studied in the presence of suspended particles and radiative transfer effects and the criteria for monotonic instability are obtained in terms of source function.

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Himachal Pradesh University
India

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