The infrared counterpart of the X-ray burster KS 1731-260

R. P. Mignani, S. Chaty, I. F. Mirabel, S. Mereghetti

Research output: Contribution to journalArticlepeer-review

Abstract

We present JK′ infrared images of the X-ray transient KS 1731-260, obtained in 1997 and in 1998 with IRAC2b at the ESO/MPI 2.2-m telescope at La Silla. Using as a reference the recent Chandra position, we confirm the identification of the X-ray source with the previously proposed counterpart (Wijnands et al. 2001b), for which we measure J = 17.32 ± 0.2 and K′ = 16.36 ± 0.18. The source was entering a low X-ray state at the epoch of our observations, and the accretion disk was still dominating the infrared flux. Indeed, when compared with the only published magnitudes in the J-band (Orosz et al. 2001), obtained with the source in quiescence, our photometry confirms the fading of the counterpart during the decay of the RXTE/ASM lightcurve.

Original languageEnglish
Pages (from-to)L11-L14
JournalAstronomy and Astrophysics
Volume389
Issue number1
DOIs
Publication statusPublished - 1 Jan 2002
Externally publishedYes

Keywords

  • KS 1731-260
  • X-ray binaries

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