Luminous X-ray sources in spiral and star-forming galaxies

被引：4

作者：

Ward, M ^{[1
]}

机构：

[1] Univ Leicester, Dept Phys & Astron, X Ray & Observ Astron Grp, Leicester LE1 7RH, Leics, England

来源：

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 2002年 / 360卷 / 1798期

关键词：

galaxies; X-rays; binaries; supernova remnants; black holes;

D O I：

10.1098/rsta.2002.1049

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

For studies of discrete X-ray source populations in nearby galaxies, high spatial resolution is a key to making progress. Now, for the first time, using the Chandra X-ray observatory, we are able to study these source populations in detail for galaxies beyond M31 and our local group galaxies. Analysis of accretion-driven and supernova-related discrete sources provides a new perspective oil the evolution of galactic stellar populations, as well as giving insights into the physical mechanisms operating in individual cases. A particularly intriguing area, which we are only just beginning to address, is the nature of the most X-ray-luminous sources that are being discovered in many spiral and star-forming galaxies.

引用

页码：1991 / 2003

页数：13

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