Cataclysmic Variables: Structure and Evolution
1994 ◽
Vol 147
◽
pp. 420-442
Keyword(s):
AbstractI discuss the structure and evolution of cataclysmic variables, with a particular emphasis on the influence of the physics used in calculating the internal structure of the secondary. The available observational data is very rich, and can, in principle, be used to constrain the stellar physics. It is found that, in order to explain the lack of systems with periods in the range 2 – 3 hr, it is required that main sequence star become convective for masses below 0.3 M⊙. This has little consequences on the equation of state, but constrains the opacities and the treatment of subphotospheric layers.
2000 ◽
Vol 176
◽
pp. 443-443
Keyword(s):
2017 ◽
Vol 468
(3)
◽
pp. 3342-3346
Keyword(s):
1979 ◽
Vol 53
◽
pp. 520-520
2004 ◽
Vol 194
◽
pp. 101-103
Keyword(s):
1976 ◽
Vol 32
◽
pp. 49-55
◽
2019 ◽
Vol 15
(S354)
◽
pp. 189-194
2010 ◽
Vol 27
(1)
◽
pp. 010401
◽
2013 ◽
Vol 768
(1)
◽
pp. 74
◽
Keyword(s):
2007 ◽
Vol 3
(S246)
◽
pp. 291-300
◽
Keyword(s):