The stability of massive stars
1994 ◽
Vol 162
◽
pp. 73-74
Keyword(s):
An investigation of the stability properties of stellar models describing massive stars is motivated observationally by the necessity to explain the observed Humphreys - Davidson (HD) limit and the variability of the most massive stars known, i.e. the existence of luminous blue variables (LBVs). Theoretically, a determination of the upper mass limit for stable stellar objects together with its physical explanation and interpretation is of fundamental interest.
1986 ◽
Vol 116
◽
pp. 45-59
Keyword(s):
2012 ◽
Vol 10
(H16)
◽
pp. 51-79
◽
Keyword(s):
1943 ◽
Vol 3
(4)
◽
pp. 541-545
◽