Stellar-mass black-hole models at Eddington luminosity

被引：0

作者：

Okuda, T ^{[1
]}

机构：

[1] Hokkaido Univ, Hokodate Coll, Hakodate, Hokkaido 0408567, Japan

来源：

PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT | 2004年 / 155期

关键词：

D O I：

暂无

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Black-hole accretion disk models with 3 and 15 Eddington critical accretion rates are examined by two-dimensional radiation hydrodynamic calculations. The numerical results show that, the super-Eddington model with 15 Eddington critical rate can explain well the small collimation degree of the jets and the high mass-outflow rate estimated for SS 433.

引用

页码：401 / 402

页数：2

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