Accretion disks around compact objects and protosteelar objects

被引:0
作者
Okuda, T [1 ]
Fujita, M [1 ]
机构
[1] Hokkaido Univ Educ, Hakodate Coll, Hakodate, Hokkaido 0408567, Japan
来源
NUMERICAL ASTROPHYSICS | 1999年 / 240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
Two-dimensional accretion disks around a neutron star near Eddington luminosity and an FU Ori object during eruptions are examined. In both cases convection plays an important role in vertical energy transport and matter accretion onto the central star. The neutron star model is applicable to SS 433 and the protostar model suggests a new observational appearance to an FU Ori object.
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页码:241 / 242
页数:2
相关论文
共 4 条
[1]   SLIM ACCRETION DISKS [J].
ABRAMOWICZ, MA ;
CZERNY, B ;
LASOTA, JP ;
SZUSZKIEWICZ, E .
ASTROPHYSICAL JOURNAL, 1988, 332 (02) :646-658
[2]  
KLEY W, 1989, ASTRON ASTROPHYS, V208, P98
[3]   A FLUX-LIMITED DIFFUSION-THEORY [J].
LEVERMORE, CD ;
POMRANING, GC .
ASTROPHYSICAL JOURNAL, 1981, 248 (01) :321-334
[4]   Two-dimensional accretion disk models: Inner accretion disks of FU Orionis objects [J].
Okuda, T ;
Fujita, M ;
Sakashita, S .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1997, 49 (06) :679-697