The Conditions of Occurrence for the Instability of a Stellar Shell Source

Details The Conditions of Occurrence for the Instability of a Stellar Shell Source The Conditions of Occurrence for the Instability of a Stellar Shell Source

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987acaps...7...33h&link_type=abstract

Acta Astrophysica Sinica, Vol. 7:1, P. 33, 1987

Astronomy and Astrophysics

Astrophysics

Scientific paper

Based on the method proposed by A. Weigert for discussing when the instability will occur in the thermonuclear source of a star, the conditions of the occurrence of the instability phenomenon (also known as thermal pulsation) in a shell source are derived. The results show that the instability phenomenon appears when the shell source is quite thin and the ratio of its thickness to the radius is less than 0.37.

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