2007MNRAS.382L..43S

Query : 2007MNRAS.382L..43S

2007MNRAS.382L..43S - Mon. Not. R. Astron. Soc., 382, L43-L47 (2007/November-3)

Neutron star cooling after deep crustal heating in the X-ray transient KS 1731-260.

SHTERNIN P.S., YAKOVLEV D.G., HAENSEL P. and POTEKHIN A.Y.

Abstract (from CDS):

We simulate the cooling of the neutron star in the X-ray transient KS 1731-260 after the source returned to quiescence in 2001 from a long (≳12.5 yr) outburst state. We show that the cooling can be explained assuming that the crust underwent deep heating during the outburst stage. In our best theoretical scenario the neutron star has no enhanced neutrino emission in the core, and its crust is thin, superfluid, and has the normal thermal conductivity. The thermal afterburst crust-core relaxation in the star may not be over.

Abstract Copyright: 2007 The Authors. Journal compilation © 2007 RAS

Journal keyword(s): stars: neutron - X-rays: individual: KS 1731-260

Simbad objects: 2

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Number of rows : 2
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 MXB 1658-298 LXB 17 02 06.54 -29 56 44.1 18.35 18.75 18.3     ~ 381 0
2 KS 1731-260 LXB 17 34 13.46 -26 05 18.6       22.8 20.9 ~ 437 0

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