Multi-Wavelength Study of High Mass X-ray Binaries

被引：0

作者：

Chaty, S. ^{[1
]}

机构：

[1] Univ Paris Diderot, Lab AIM, CNRS, UMR 7158,CEA,DSM,Irfu Serv Astrophy,CEA Saclay, FR-91191 Gif Sur Yvette, France

来源：

INTERNATIONAL CONFERENCE ON BINARIES: IN CELEBRATION OF RON WEBBINK'S 65TH BIRTHDAY | 2010年 / 1314卷

关键词：

X-ray binaries; supergiant stars; IGR J16318-4848; COMPANION STAR; STELLAR WINDS; NEUTRON-STAR; TRANSIENT; EVOLUTION; CATALOG; IGR-J16318-4848; J17544-2619;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The INTEGRAL satellite has revealed a major population of supergiant High Mass X-ray Binaries in our Galaxy, revolutionizing our understanding of binary systems and their evolution. This population, constituted of a compact object orbiting around a massive and luminous supergiant star, exhibits unusual properties, either being extremely absorbed, or showing very short and intense flares. An intensive set of multi-wavelength observations has led us to reveal their nature, and to show that these systems are wind-fed accretors, closely related to massive star-forming regions. In this paper I describe the characteristics of these sources, showing that this newly revealed population is closely linked to the evolution of active and massive OB stars with a compact companion. The last section emphasizes the formation and evolution of such High Mass X-ray Binaries hosting a supergiant star.

引用

页码：277 / 284

页数：8

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