INTEGRAL and Swift observations of the Be X-ray binary 4U 1036-56 (RX   J1037.5-5647) and its possible relation with gamma-ray transients
  We present timing, spectral, and long-term temporal analysis of the high mass X-ray binary (HMXB) 4U 1036-56 using INTEGRAL and Swift observations. We show that it is a weak hard X-ray source spending a major fraction of the time in quiescence, and only occasionally characterized by X-ray outbursts. The outburst activity we report here lasts several days, with a dynamic range spanned by the luminosity in quiescence and in outburst as high as ~30. We report the detection of pulse period at 854.75+/-4.39 s during an outburst, which is consistent with previous measurements. Finally, we analyze the possibility of 4U 1036--56's association with the unidentified transient gamma-ray sources AGL J1037--5708 & GRO J1036--55, as prompted by its positional correlation. 
Jian Li, Diego F. Torres, Shu Zhang, Alessandro Papitto, Yupeng Chen,   Jian-Min Wang
astro-ph.HE