X-ray wind tomography of the highly absorbed HMXB IGR J17252–3616

Context. About ten persistently highly absorbed super-giant high-mass X-ray binaries (sgHMXB) have been discovered by INTEGRAL as bright hard X-ray sources lacking bright X-ray counterparts. Besides IGR J16318-4848, which has peculiar characteristics, the other members of this family share many prop...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2011-02, Vol.526, p.A62
Hauptverfasser:	Manousakis, A., Walter, R.
Format:	Artikel
Sprache:	eng
Schlagworte:	3616 Astronomy Earth, ocean, space Exact sciences and technology outflows pulsars: individual: IGR J17252 stars: winds supergiants X-rays: binaries
Online-Zugang:	Volltext
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