Multiwavelength observations of 1RXH J173523.7−354013: revealing an unusual bursting neutron star.

On 2008 May 14, the Burst Alert Telescope onboard the Swift mission triggered on a type-I X-ray burst from the previously unclassified ROSAT object 1RXH , establishing the source as a neutron star X-ray binary. We report on X-ray, optical and near-infrared observations of this system. The X-ray burst had a duration of ∼2 h and belongs to the class of rare, intermediately long type-I X-ray bursts. From the bolometric peak flux of , we infer a source distance of . Photometry of the field reveals an optical counterpart that declined from during the X-ray burst to thereafter. Analysis of post-burst Swift/X-ray Telescope observations as well as archival XMM–Newton and ROSAT data suggests that the system is persistent at a 0.5–10 keV luminosity of . Optical and infrared photometry together with the detection of a narrow emission line (full width at half maximum , equivalent width ) in the optical spectrum confirms that 1RXH is a neutron star low-mass X-ray binary. The emission demonstrates that the donor star is hydrogen rich, which effectively rules out that this system is an ultracompact X-ray binary. [ABSTRACT FROM AUTHOR]