X1908+075: A Late O-Type Supergiant with a Neutron Star Companion

Details X1908+075: A Late O-Type Supergiant with a Neutron Star Companion X1908+075: A Late O-Type Supergiant with a Neutron Star Companion

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.304..295m&link_type=abstract

Astrophysics and Space Science, Volume 304, Issue 1-4, pp. 295-297

Astronomy and Astrophysics

Astrophysics

Stars: Early-Type, Infrared: Stars, X-Rays: Binaries, X-Rays: Individual: X1908+075

Scientific paper

X1908 + 075 is a highly-absorbed Galactic X-ray source likely made up of a pulsar accreting wind material from a massive companion. We have used near-IR photometric data complemented by follow-up spectroscopy to identify the likely counterpart to this X-ray source and to assign a spectral type O7.5 9.5 If to the primary. Further details can be found in Morel and Grosdidier (2005).

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