SIMBAD references

2008A&A...492..163R - Astronomy and Astrophysics, volume 492, 163-166 (2008/12-2)

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

RAHOUI F. and CHATY S.

Abstract (from CDS):

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 uncertain - led to the conclusion that the source was probably a 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 and discriminate between a BeXB and a SFXT nature for this 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, probably a B0.5a, and that its distance is about 3-4kpc. The early-B supergiant nature of its companion star, as well as its fast X-ray transient activity indicate that IGR J18483-0311 has an SFXT nature. 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.

Abstract Copyright:

Journal keyword(s): infrared: stars - X-rays: binaries - stars: individual: IGR J18483-0311 - binaries: general - supergiants - stars: fundamental parameters

CDS comments: Paragraph 2.1 The four photometric standard stars are probably misprint for PG 1657+078, A, B, C.

Simbad objects: 8

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2020.09.19-18:48:18

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