2001MNRAS.321..327K

Query : 2001MNRAS.321..327K

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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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 2E 0035.4-7229 XB* 00 37 19.6683991960 -72 14 13.187852739   20.0 20.2     ~ 104 0
2 RX J0537.6-7033 XB* 05 37 43.0 -70 34 15           ~ 33 0
3 V* V1033 Sco HXB 16 54 00.1423963019 -39 50 44.761701340       16.14   F3-6IV 1980 0
4 V* V1341 Cyg LXB 21 44 41.1544345272 +38 19 17.066570988 15.00 15.13 14.68 15.00   A9III 1229 1

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