IGR J18483-0311: a new intermediate supergiant fast X-ray transient

TL;DR

This paper identifies IGR J18483-0311's companion as an early-B supergiant, suggesting it is an intermediate supergiant fast X-ray transient with unique outburst characteristics, bridging classical SFXTs and SGXBs.

Contribution

The study provides the first detailed spectral and physical characterization of IGR J18483-0311's companion star, clarifying its nature as an intermediate SFXT.

Findings

Companion star is an early-B supergiant, likely B0.5Ia.

Distance estimated at 3-4 kpc.

Source exhibits properties of an intermediate SFXT.

Abstract

IGR J18483-0311 is a high-mass X-ray binary recently discovered by INTEGRAL. Its periodic fast X-ray transient activity and its position in the Corbet diagram - although ambiguous - led to the conclusion that the source was a likely Be/X-ray binary (BeXB), even if a supergiant fast X-ray transient (SFXT) nature could not be excluded. We aimed at identifying the companion star of IGR J18483-0311 to discriminate between the BeXB and the SFXT nature of the source. Optical and near-infrared photometry, as well as near-infrared spectroscopy of the companion star were performed to identify its spectral type. We also assembled and fitted its broad-band spectral energy distribution to derive its physical parameters. We show that the companion star of IGR J18483-0311 is an early-B supergiant, likely a B0.5Ia, and that its distance is about 3-4 kpc. The early-B supergiant nature of its companion star, as well as its fast X-ray transient activity point towards an SFXT nature of IGR J18483-0311. Nevertheless, the long duration and the periodicity of its outbursts, as well as its high level of quiescence, are consistent with IGR J18483-0311 being an intermediate SFXT, in between classical supergiant X-ray binaries (SGXBs) characterised by small and circular orbits, and classical SFXTs with large and eccentric orbits.