[MG2005] A , the SIMBAD biblio

2005MNRAS.356..665M - Mon. Not. R. Astron. Soc., 356, 665-670 (2005/January-2)

Near-infrared identification of the counterpart to X1908+075: a new OB-supergiant X-ray binary.


Abstract (from CDS):

We report the near-infrared (near-IR) identification of the likely counterpart to X1908+075, a highly absorbed Galactic X-ray source recently suspected to belong to the rare class of OB supergiant-neutron star binary systems. Our JHKs-band imaging of the field reveals the existence within the X-ray error boxes of a near-IR source consistent with an early-type star lying at d∼ 7 kpc and suffering AV∼ 16 mag of extinction, the latter value being in good agreement with the hydrogen column density derived from modelling of the X-ray spectrum. Our follow-up, near-IR spectroscopic observations confirm the nature of this candidate and lead to a late O-type supergiant classification, thereby supporting the identification of a new Galactic OB-supergiant X-ray binary.

Abstract Copyright: 2004 RAS

Journal keyword(s): stars: early-type - infrared: stars - X-rays: binaries - X-rays: individual: X1908+075

Nomenclature: Fig.1, Table 1: [MG2005] A (Nos A-C).

Simbad objects: 14

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