New elements for three eclipsing X-ray binary systems: HZ Herculis, Centaurus X-3, and Vela X-1

被引：1

作者：

Al-Wardat, MAS ^{[1
]}

Al-Naimiy, HM ^{[1
]}

Barghouthi, IA ^{[1
]}

Sabat, HA ^{[1
]}

机构：

[1] Al Al Bayt Univ, Higher Inst Astron & Space Sci, Al Mafraq, Jordan

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1998年 / 260卷 / 03期

关键词：

D O I：

10.1023/A:1001714812242

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A contribution to the theoretical analysis of eclipsing x-ray binary systems and the calculation of physical and geometrical elements, are represented. The principle of this work is to make fitting between the observational light curve and the synthetic light curve built up in accordance with the Roche model, and to consider the elements of the best fitting as new elements. This method were applied to three systems, there are: (i) HZ Herculis (Hercules X-1). (ii) Krzemenski's star (Centaurus X-3). (iii) HD 77851 (Vela X-1). Finally, the mass-luminosity relation and the H-R diagram for the optical components of the three systems, have been plotted and studied.

引用

页码：335 / 345

页数：11

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