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Simulating the X-ray evolution of late-type galaxies with population synthesis

Published online by Cambridge University Press:  21 February 2013

Zhao-yu Zuo  and
Xiang-dong Li
Zhao-yu Zuo
Affiliation:
Dept. of Physics, School of Science, Xi'an Jiaotong University, Xi'an 710049, China
Xiang-dong Li
Affiliation:
Dept. of Astronomy, Nanjing University, Nanjing 210093, China email: zuozyu@mail.xjtu.edu.cn, lixd@nju.edu.cn
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Abstract

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Using an evolutionary population synthesis code, we modeled the global emission of X-ray binaries in late-type galaxies, its relations with other physical properties (i.e., optical luminosity, stellar mass, etc.) of the galaxies, and their evolution with redshift over the cosmic history, which may be investigated further by future high-resolution X-ray and optical observations.

Keywords

Stellar evolutioncompact starsX-ray binaries
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 375 - 376
Copyright
Copyright © International Astronomical Union 2013

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