Cepheid Evolution with Pulsationally-Driven Mass Loss
1989 ◽
Vol 111
◽
pp. 252-252
◽
AbstractWe have studied the effects of a pulsationally-driven wind on Cepheid evolution. Mass loss due to the wind, which occurs only when the star is crossing the Cepheid instability strip, is a function of luminosity and radius. We have investigated the evolution of 4, 5, 6, 7 and 8 M⊙ stars using the updated 12C(α,γ) 16O rates.
2014 ◽
Vol 9
(S307)
◽
pp. 224-225
Keyword(s):
2016 ◽
Vol 152
(6)
◽
pp. 200
◽
Mass-Loss During the RR Lyrae Phase of the HB: Mass Dispersion on the HB and RR Lyrae Period Changes
1993 ◽
Vol 139
◽
pp. 312-312
1993 ◽
Vol 139
◽
pp. 284-284
Keyword(s):
1979 ◽
Vol 46
◽
pp. 318-321
Keyword(s):
Keyword(s):