STRUCTURED CORONAE OF ACCRETION DISKS

被引：650

作者：

GALEEV, AA ^{[1
]}

ROSNER, R ^{[1
]}

VAIANA, GS ^{[1
]}

机构：

[1] IST & OSSERVATORIO ASTRON, PALERMO, ITALY

来源：

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

页码：318 / 326

页数：9

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
BLUMENTH.GR
TUCKER, WH
[J]. 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
EARDLEY, DM
LIGHTMAN, AP
[J]. 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
FORSLUND, DW
[J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1970, 75 (01): : 17 - +