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 language | English |
|---|---|
| Pages (from-to) | L11-L14 |
| Journal | Astronomy and Astrophysics |
| Volume | 389 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Jan 2002 |
| Externally published | Yes |
Keywords
- KS 1731-260
- X-ray binaries