2000MNRAS.314..290C

Query : 2000MNRAS.314..290C

2000MNRAS.314..290C - Mon. Not. R. Astron. Soc., 314, 290-294 (2000/May-2)

The SMC X-ray transient XTE J0111.2-7317: a Be/X-ray binary in a supernova remnant ?

COE M.J., HAIGH N.J. and REIG P.

Abstract (from CDS):

We report observations which confirm the identity of the optical/IR counterpart to the Rossi X-ray Timing Explorer transient source XTE J0111.2-7317. The counterpart is suggested to be a B0-B2 star (luminosity class III-V) showing an IR excess and strong Balmer emission lines. The distance derived from reddening and systemic velocity measurements puts the source in the Small Magellanic Cloud (SMC). Unusually, the source exhibits an extended asymmetric Hα structure.

Abstract Copyright: 2000, Royal Astronomical Society

Journal keyword(s): binaries: close - stars: emission-line, Be - pulsars: general - infrared: stars - X-rays: stars

Simbad objects: 5

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Number of rows : 5
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 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 RX J0105.1-7211 HXB 01 05 09.941 -72 11 47.00   15.62 15.63 18.3   B1-B2III-V 54 1
3 RX J0111.2-7317 HXB 01 11 08.5770101712 -73 16 46.308129384 14.40 15.42 15.52   15.29 B0.5-1Ve 76 0
4 [MA93] 1845 HXB 01 17 40.1630558064 -73 30 50.523690888 13.30 14.14 14.18   14.09 B1-3(II)e 63 0
5 V* GP Vel HXB 09 02 06.8608812864 -40 33 16.899168060 6.85 7.37 6.87 6.31 6.05 B0.5Ia 1588 0

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