STRUCTURED CORONAE OF ACCRETION DISKS

被引:659
作者
GALEEV, AA [1 ]
ROSNER, R [1 ]
VAIANA, GS [1 ]
机构
[1] IST & OSSERVATORIO ASTRON, PALERMO, ITALY
关键词
D O I
10.1086/156957
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:318 / 326
页数:9
相关论文
共 25 条
[1]  
[Anonymous], 1975, RAD PROCESSES ASTROP
[2]  
Athay R. G., 1976, SOLAR CHROMOSPHERE C
[3]  
BISNOVATYIKOGAN GS, 1977, ASTRON ASTROPHYS, V59, P111
[4]   COMPACT X-RAY SOURCES [J].
BLUMENTH.GR ;
TUCKER, WH .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1974, 12 :23-46
[5]  
BOLT E, 1975, P INT C XRAYS SPACE
[6]  
BRAGINSKII SN, 1963, REV PLASMA PHYS, V1, P249
[7]  
Eardley D. M., 1978, Comments on Astrophysics. Comments on Modern Physics: Part C, V7, P151
[8]   MAGNETIC VISCOSITY IN RELATIVISTIC ACCRETION DISKS [J].
EARDLEY, DM ;
LIGHTMAN, AP .
ASTROPHYSICAL JOURNAL, 1975, 200 (01) :187-203
[9]  
FELTEN JE, 1972, ASTRON ASTROPHYS, V17, P216
[10]   INSTABILITIES ASSOCIATED WITH HEAT CONDUCTION IN SOLAR WIND AND THEIR CONSEQUENCES [J].
FORSLUND, DW .
JOURNAL OF GEOPHYSICAL RESEARCH, 1970, 75 (01) :17-+