Supercritical winds from cool 'canonical' stars caused by evolution on the Main Sequence

Details Supercritical winds from cool 'canonical' stars caused by evolution on the Main Sequence Supercritical winds from cool 'canonical' stars caused by evolution on the Main Sequence

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119...51v&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Statistics

Computation

Cool Stars, Main Sequence Stars, Stellar Evolution, Stellar Winds, Supercritical Flow, Acoustic Velocity, Computational Astrophysics, Radii, Stellar Temperature, Unsteady Flow

Scientific paper

Even the very slow expansion of a star's radius due to evolution on the main sequence is shown to be supercritical for cool stars without coronae. Since steady spherically-symmetric supercritical solutions are theoretically impossible, unsteady supercritical solutions are studied. It is seen that smooth sonic transitions are possible in the unsteady case, but they are accompanied by enhancement of pressure over the critical values.

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