THERMAL EQUILIBRIA OF ACCRETION DISKS

被引：624

作者：

ABRAMOWICZ, MA

CHEN, XM

KATO, S

LASOTA, JP

REGEV, O

机构：

[1] CHALMERS UNIV TECHNOL,S-41296 GOTHENBURG,SWEDEN

[2] TECHNION ISRAEL INST TECHNOL,DEPT PHYS,IL-32000 HAIFA,ISRAEL

[3] KYOTO UNIV,DEPT ASTRON,SAKYO KU,KYOTO 60601,JAPAN

[4] CNRS,UPR 176,F-92195 MEUDON,FRANCE

[5] OBSERV PARIS,SECT MEUDON,DARC,F-92195 MEUDON,FRANCE

来源：

ASTROPHYSICAL JOURNAL | 1995年 / 438卷 / 01期

关键词：

ACCRETION; ACCRETION DISKS; INSTABILITIES;

D O I：

10.1086/187709

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that most of hot, optically thin accretion disk models that ignore advective cooling are not self-consistent. We have found new types of optically thin disk solutions where cooling is dominated by radial advection of heat. These new solutions are thermally and viscously stable.

引用

页码：L37 / L39

页数：3

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