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The dark side of supergiant High-Mass X-ray Binaries

Published online by Cambridge University Press:  30 December 2019

Sylvain Chaty ,
Francis Fortin Open the ORCID record for Francis Fortin [Opens in a new window] ,
Federico García Open the ORCID record for Federico García [Opens in a new window]  and
Federico Fogantini
Sylvain Chaty
Affiliation:
AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France email: [email protected]
Francis Fortin
Affiliation:
AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France email: [email protected]
Federico García
Affiliation:
AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France email: [email protected]
Federico Fogantini
Affiliation:
Instituto Argentino de Radioastronomía (CCT-La Plata, CONICET, CICPBA), C.C. No. 5, 1894 Villa Elisa, and Facultad de Ciencias Astronómicas y Geofisicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina
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Abstract

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. High Mass X-ray Binaries (HMXB) have been revealed by a wealth of multi-wavelength observations, from X-ray to optical and infrared domain. After describing the 3 different kinds of HMXB, we focus on 3 HMXB hosting supergiant stars: IGR J16320-4751, IGR J16465-4507 and IGR J16318-4848, respectively called “The Good”, “The Bad” and “The Ugly”. We review in these proceedings what the observations of these sources have brought to light concerning our knowledge of HMXB, and what part still remains in the dark side. Many questions are still pending, related to accretion processes, stellar wind properties in these massive and active stars, and the overall evolution due to transfer of mass and angular momentum between the companion star and the compact object. Future observations should be able to answer these questions, which constitute the dark side of HMXB.

Keywords

(stars:) binaries (including multiple): closecircumstellar matterearly-typeemission-lineBestars: neutronsupergiantswindsoutflows(ISM:) dustextinctioninfrared: starsX-rays: binaries: IGR J16320-4751IGR J16465-4507 and IGR J16318-4848
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 161 - 169
Copyright
© International Astronomical Union 2019 

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