The fluctuation theory of mass loss - Application to the evolution of massive stars

Details The fluctuation theory of mass loss - Application to the evolution of massive stars The fluctuation theory of mass loss - Application to the evolution of massive stars

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....95..202a&link_type=abstract

Astronomy and Astrophysics, vol. 95, no. 1, Feb. 1981, p. 202, 203. Fonds de la Recherche Fondamentale Collective

Astronomy and Astrophysics

Astrophysics

11

Fluctuation Theory, Stellar Evolution, Stellar Mass Ejection, Supermassive Stars, Hertzsprung-Russell Diagram, Hot Stars, Red Giant Stars

Scientific paper

It is shown that the application of the fluctuation theory of the
stellar mass loss in computing the evolution of massive stars leads to
an explanation of certain features in the H-R diagrams. These include
the absence of highly luminous red supergiants, the rate blow-off
phenomenon, and the existence of single WR(N) stars.

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