VO332+53爆发时气体流的结构

计算物理 ›› 1997, Vol. 14 ›› Issue (S1): 581-583.

VO332+53爆发时气体流的结构

宓国柱¹, 沈金英²

1. 南京航空航天大学理学院, 210016;
2. 南京大学国际商学院, 210008

收稿日期:1997-03-03 修回日期:1997-05-08 出版日期:1997-12-25 发布日期:1997-12-25

THE STRUCTURE OF GAS OUTFLOW DURING THE OUTBURSTS FROM VO332+53

Mi Guozhu¹, Shen Jinying²

1. College of Science, Nanjing University of Aeronautics and Astronautics, 210016;
2. School of International Business, Nanjing University, 210008

Received:1997-03-03 Revised:1997-05-08 Online:1997-12-25 Published:1997-12-25

摘要/Abstract

摘要： 运用气盘和缓慢加速星风的混合模型,计算了由Be星和中子星组成的双星系统的X射线光度的变化,与VO332+53的观测资料作了较好的拟合。

关键词: Be星, 星风, X射线双星, X射线爆发

Abstract: A hybrid model consisting of a gas disc plus a slowly accelerating wind is used to calculate the X-ray light curves in a Be and neutron star binary.The observational data of VO332+53 are coincident with some of them.

Key words: Be star, stellar wind, X-ray binary, X-ray burst

中图分类号:

P142.6

宓国柱, 沈金英. VO332+53爆发时气体流的结构[J]. 计算物理, 1997, 14(S1): 581-583.

Mi Guozhu, Shen Jinying. THE STRUCTURE OF GAS OUTFLOW DURING THE OUTBURSTS FROM VO332+53[J]. CHINESE JOURNAL OF COMPUTATIONAL PHYSICS, 1997, 14(S1): 581-583.

[1]	刘门全, 罗志全, 彭秋和, 谢佐恒. 压强梯度对Ws12M_⊙模型瞬时爆发能量的影响[J]. 计算物理, 2006, 23(4): 494-498.
[2]	张锁春. 超新星铁星核区对流不稳定的数值模拟[J]. 计算物理, 1997, 14(S1): 545-546.
[3]	王贻仁, 谢佐恒, 汪惟中, 张锁春. Ⅱ型超新星铁星核质量对瞬发爆炸的影响[J]. 计算物理, 1997, 14(S1): 547-549.