Reference : X1908+075: A Late O-Type Supergiant with a Neutron Star Companion
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/31327
X1908+075: A Late O-Type Supergiant with a Neutron Star Companion
English
Morel, Thierry [Katholieke Universiteit Leuven, Departement Natuurkunde en Sterrenkunde, Instituut voor Sterrenkunde, Celestijnenlaan 200D, 3001 Leuven, Belgium > > > >]
Grosdidier, Yves [Department of Physics, McGill University]
1-Aug-2006
Astrophysics & Space Science
Springer Science & Business Media B.V.
304
295-297
Yes (verified by ORBi)
International
0004-640X
Dordrecht
The Netherlands
[en] Stars: early-type ; Infrared: stars ; X-rays: binaries ; X-rays: individual: X1908+075
[en] 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).
http://hdl.handle.net/2268/31327
10.1007/s10509-006-9135-7
http://adsabs.harvard.edu/abs/2006Ap%26SS.304..295M

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