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

@article{Morel2005NearinfraredIO,
  title={Near‐infrared identification of the counterpart to X1908+075: a new OB‐supergiant X‐ray binary},
  author={Thierry Morel and Yves Grosdidier},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2005},
  volume={356},
  pages={665-670}
}
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… 

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