Stability of the sun against nonradial thermal modes

Details Stability of the sun against nonradial thermal modes Stability of the sun against nonradial thermal modes

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..263s&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 1-2, May 1980, p. 263, 264.

Physics

2

Solar Physics, Stellar Models, Thermal Stability, Abundance

Scientific paper

The stability of solar models against nonspherical thermal modes is investigated using the stability condition derived by Gabriel and Noels (1976). The standard solar models are found to be stable against a nonradial thermal mode even when a chemically inhomogeneous zone exists. This conclusion is consistent with the result of Rosenbluth and Bahcall (1973).

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