The near-IR counterpart to the high-mass X-ray binary X1908+075

Details The near-IR counterpart to the high-mass X-ray binary X1908+075 The near-IR counterpart to the high-mass X-ray binary X1908+075

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..291....1m&link_type=abstract

The Astronomer's Telegram, #291

Astronomy and Astrophysics

Astronomy

Infra-Red, X-Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

We report the 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 (Wen et al. 2000, ApJ, 532, 1119; Levine et al. 2004, ApJ, submitted, astro-ph/0404428). The Einstein and HEAO 1 satellites have localized this X-ray source with an uncertainty of about 50''.

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