X-ray observations of SS 433 with ASCA

被引：0

作者：

Kotani, T ^{[1
]}

Kawai, N ^{[1
]}

Matsuoka, M ^{[1
]}

Brinkmann, W ^{[1
]}

机构：

[1] RIKEN, Cos Rad Lab, Wako, Saitama 35101, Japan

来源：

ACCRETION PHENOMENA AND RELATED OUTFLOWS: IAU COLLOQUIUM 163 | 1997年 / 121卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

SS 433 has been observed with ASCA for three years since the launch in 1993. The excellent energy resolution of ASCA revealed the Doppler-shifted emission lines from the both jets, though it had been generally accepted that the X-ray emitting region of the receding jet is hidden behind the accretion disk. Thus the estimation on the properties of the X-ray jet, such as length, temperature, and mass outflow rate, should be revised in accordance with the ASCA data. Modeling the jet as a radiating ballistic plasma, we determined these quantities. It is also tried to determine the mass of the system from a data covering an eclipse.

引用

页码：370 / 374

页数：5

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