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The evolutionary history of BE/X-ray binaries

Published online by Cambridge University Press:  04 August 2017

G.M.H.J. Habets
G.M.H.J. Habets*
Affiliation:
Astronomical Institute, University of Amsterdam, Roetersstraat 15, 1018 WB Amsterdam

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A 2.5 M⊙ helium star remnant of a Case B mass transfer is evolved to off-centre neon ignition and a second mass transfer phase, Case BB, is explored. The model for the formation of Be/X-ray binaries by mass-transfer dominated evolution in an intermediate mass binary is confirmed.

Information

Type
III. BINARITY, PULSATION, ROTATION AND MIXING
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984, pp. 399 - 402
Copyright
Copyright © Reidel 1984 

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