Fundamental parameters of low mass X-ray binaries II: X-ray persistent systems

被引：0

作者：

Casares, Jorge ^{[1
]}

Charles, Phil ^{[1
]}

机构：

[1] Inst Astrofis Canarias, Tenerife 38200, Spain

来源：

SPECTRA AND TIMING OF COMPACT X-RAY BINARIES | 2006年 / 38卷 / 12期

关键词：

binaries : close; X-rays : binaries; stars : neutron; accretion : accretion discs;

D O I：

暂无

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The determination of fundamental parameters in X-ray luminous (persistent) X-ray binaries has been classically hampered by the large optical luminosity of the accretion disc. New methods, based on irradiation of the donor star and burst oscillations, provide the opportunity to derive dynamical information and mass constraints in many persistent systems for the first time. These techniques are here reviewed and the latest results presented. (c) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：2731 / +

页数：3

共 38 条

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[2]

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[3]

Augusteijn T, 1998, ASTRON ASTROPHYS, V332, P561

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