Uncertainties in the Position of the β Cephei Instability Strip in the HR Diagram
1995 ◽
Vol 155
◽
pp. 291-292
AbstractWe discuss the sensitivity of the theoretical B star instability domains to the heavy element abundance Z, the adopted metal mixture, the assumed overshooting from stellar convective cores and the choice of the opacity data.
1996 ◽
Vol 152
◽
pp. 217-222
Keyword(s):
1977 ◽
Vol 42
◽
pp. 242-273
◽
Keyword(s):
2012 ◽
Vol 10
(H16)
◽
pp. 247-248
◽
Keyword(s):
Keyword(s):
1993 ◽
Vol 137
◽
pp. 651-653
◽
2002 ◽
Vol 393
(3)
◽
pp. L95-L98
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