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26 April 2024
 
  » arxiv » astro-ph/9903282

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The X-ray Transient XTE J2012+381
R.I. Hynes ; P. Roche ; P.A. Charles ; M.J. Coe ;
Date 18 Mar 1999
Journal Mon.Not.Roy.Astron.Soc. 305 (1999) L49
Subject astro-ph
AffiliationSussex), P.A. Charles (Oxford), M.J. Coe (Southampton
AbstractWe present optical and infrared observations of the soft X-ray transient (SXT) XTE J2012+381 and identify the optical counterpart with a faint red star heavily blended with a brighter foreground star. The fainter star is coincident with the radio counterpart and appears to show weak H alpha emission and to have faded between observations. The RXTE/ASM lightcurve of XTE J2012+381 is unusual for an SXT in that after an extended linear decay, it settled into a plateau state for about 40 days before undergoing a weak mini-outburst. We discuss the nature of the object and suggest similarities to long orbital period SXTs.
Source arXiv, astro-ph/9903282
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