A note on the conditions for SSD-ADAF transitions

被引：29

作者：

Abramowicz, MA ^{[1
]}

Igumenshchev, IV

Lasota, JP

机构：

[1] Gothenburg Univ, Dept Astron & Astrophys, S-41296 Gothenburg, Sweden

[2] Chalmers Univ Technol, S-41296 Gothenburg, Sweden

[3] NORDITA, DK-2100 Copenhagen O, Denmark

[4] Russian Acad Sci, Inst Astron, Moscow 109017, Russia

[5] Observ Paris, DARC, Sect Meudon, CNRS,UPR 176, F-92195 Meudon, France

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1998年 / 293卷 / 04期

关键词：

accretion; accretion discs; convection; hydrodynamics;

D O I：

10.1046/j.1365-8711.1998.01201.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

One of the necessary matching conditions between an optically thin, hot, advectively dominated part of an accretion disc (ADAF) and the standard Shakura-Sunyaev disc (SSD) part is that the matching transition region must rotate with an orbital speed that is faster than the Keplerian one. We discuss properties of the SSD-ADAF transition in terms of a simple two-dimensional hydrodynamical model.

引用

页码：443 / 446

页数：4

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