Optical/infrared observations unveiling the formation,nature and evolution of High-Mass X-ray Binaries |
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| Authors: | Sylvain Chaty |
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| Institution: | AIM (UMR-E 9005 CEA/DSM-CNRS-Université Paris Diderot), Irfu/Service d’Astrophysique, Centre de Saclay, FR-91191 Gif-sur-Yvette Cedex, France; Institut Universitaire de France, 103 Boulevard Saint-Michel, 75005 Paris, France |
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| Abstract: | In this review I first describe the nature of the three kinds of High-Mass X-ray Binaries (HMXBs), accreting through: (i) Be circumstellar disc, (ii) supergiant stellar wind, and (iii) Roche lobe filling supergiants. |
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| Keywords: | Circumstellar matter &ndash stars: emission-line B[e] &ndash X-rays: binaries &ndash X-rays: individual (IGR J16318-4848 IGR J17544-2619) |
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