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

	Document type :	Scientific journals : Article
	Discipline(s) :	Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
	To cite this reference:	http://hdl.handle.net/2268/31327

Title :	X1908+075: A Late O-Type Supergiant with a Neutron Star Companion
Language :	English
Author, co-author :	Morel, Thierry [Katholieke Universiteit Leuven, Departement Natuurkunde en Sterrenkunde, Instituut voor Sterrenkunde, Celestijnenlaan 200D, 3001 Leuven, Belgium > > > >]
	Grosdidier, Yves [Department of Physics, McGill University]
Publication date :	1-Aug-2006
Journal title :	Astrophysics & Space Science
Publisher :	Springer Science & Business Media B.V.
Volume :	304
Pages :	295-297
Peer reviewed :	Yes (verified by ORBi)
Audience :	International
ISSN :	0004-640X
City :	Dordrecht
Country :	The Netherlands
Keywords :	[en] Stars: early-type ; Infrared: stars ; X-rays: binaries ; X-rays: individual: X1908+075
Abstract :	[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).
Permalink :	http://hdl.handle.net/2268/31327
DOI :	10.1007/s10509-006-9135-7
Other URL :	http://adsabs.harvard.edu/abs/2006Ap%26SS.304..295M

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