Maximum Mass Loss From Stars

Open Access

1 July 1967

journal article
Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society

Vol. 136 (3) , 341-346
https://doi.org/10.1093/mnras/136.3.341

Abstract

Basing the argument on simple energy considerations, an expression giving an upper bound to the rate at which stars can emit material is obtained. Using this, numerical values are found for the upper bound to the mass loss from main-sequence, giant and supergiant stars.

Keywords

MASS LOSS
GIVING
SUPERGIANT
EMIT
LOSS FROM STARS
STARS BASING
ARGUMENT ON SIMPLE

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