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Evolution of massive close binaries (1976)

Grève, J. P. ; Loore, C.

Springer

Astrophysics and space science 43 (1976), S. 35-46

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ISSN: 1572-946X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract The evolution of a binary system with components of 10M ⊙ and 8M ⊙ is computed through a case B of mass exchange. It is found that after the end of core helium burning, a second stage of mass transfer from the primary occurs. Carbon ignition is prohibited by the large neutrino losses in the degenerated core. The primary remnant, a 1.12M ⊙ star, ends as a white dwarf. A comparison with the 10M ⊙ single evolution is made.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00640553

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