SIMBAD references

2003MNRAS.344.1075C - Mon. Not. R. Astron. Soc., 344, 1075-1084 (2003/October-1)

XTE J0111.2-7317: a nebula-embedded X-ray binary in the Small Magellanic Cloud.

COE M.J., HAIGH N.J., WILSON C.A. and NEGUERUELA I.

Abstract (from CDS):

The observed characteristics of the nebulosity surrounding the Small Magellanic Cloud (SMC) high-mass X-ray binary XTE J0111.2-7317 are examined in the context of three possible nebular types: supernova remnant, bowshock and HII region. Observational evidence is presented which appears to support the interpretation that the nebulosity surrounding XTE J0111.2-7317 is an HII region. The source therefore appears to be a normal SMC Be X-ray binary (BeXRB) embedded in a locally enhanced interstellar medium which it has photoionized to create an HII region. This is supported by observations of the X-ray outburst seen with the Burst and Transient Source Experiment (BATSE) and Rossi X-ray Timing Explorer (RXTE) in 1998-1999. It exhibited characteristics typical of a giant or type II outburst in a BeXRB including large spin-up rates, LX≥ 1038 erg/cm2/s, and a correlation between spin-up rate and pulsed flux. However, the temporal profile of the outburst was unusual, consisting of two similar intensity peaks, with the first peak of shorter duration than the second.

Abstract Copyright: 2003 RAS

Journal keyword(s): stars: emmission-line, Be - X-rays: binaries

Simbad objects: 8

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2003MNRAS.344.1075C and select 'bookmark this link' or equivalent in the popup menu


2020.02.17-19:42:44

© Université de Strasbourg/CNRS

    • Contact