Mass Ejection by Highly Evolved Stars

Details Mass Ejection by Highly Evolved Stars Mass Ejection by Highly Evolved Stars

Apr 1966

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1966natur.210..510g&link_type=abstract

Nature, Volume 210, Issue 5035, pp. 510-511 (1966).

Physics

Scientific paper

THE problem of the surprisingly high abundance of galactic helium which has been observed1,2 was the stimulus for this work. This communication proposes a new mechanism for rapid mass ejection from highly evolved stars. The mechanism is effective only over a specific, relatively short period of time in the life of the star. The general problem of mass loss from stars is the subject of an excellent review by Weymann3.

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