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2001MNRAS.321..327K - Mon. Not. R. Astron. Soc., 321, 327-332 (2001/February-3)
The minimum orbital period in thermal time-scale mass transfer.
KING A.R., SCHENKER K., KOLB U. and DAVIES M.B.
Abstract (from CDS):
We show that the usual picture of supersoft X-ray binary evolution as driven by conservative thermal time-scale mass transfer cannot explain the short orbital periods of RX J0537.7-7034 (3.5h) and 1E0035.4-7230 (4.1h). Non-conservative evolution may produce such periods, but requires very significant mass loss, and is highly constrained.
Abstract Copyright: 2001, Royal Astronomical Society
Journal keyword(s): binaries: close - stars: evolution - stars: individual: 1E0035.4-7230 - stars: individual: RX J0537.7-7034 - X-rays: stars
Simbad objects: 4
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