THE COLLIMATION OF PARTICLE BEAMS FROM THICK ACCRETION DISKS

被引：95

作者：

SIKORA, M ^{[1
]}

WILSON, DB ^{[1
]}

机构：

[1] INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1981年 / 197卷 / 02期

关键词：

D O I：

10.1093/mnras/197.3.529

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The acceleration and collimation of particle beams in the funnel of thick accretion discs is studied in the approximation that the flow is optically thin. Such flows can be collimated to within - 0 . 1 radians by sufficiently thick discs. The flow cannot convert more than a small fraction of the disc's (super-Eddington) luminosity into the energy flow of a narrow beam without being optically thick. © Royal Astronomical Society.

引用

页码：529 / 541

页数：13

共 14 条

[1] KINEMATIC MODEL FOR SS433
ABELL, GO
MARGON, B
[J]. NATURE, 1979, 279 (5715) : 701 - 703
[2] ABRAMOWICZ M, 1978, ASTRON ASTROPHYS, V63, P221
[3] THICK ACCRETION DISKS WITH SUPER-EDDINGTON LUMINOSITIES
ABRAMOWICZ, MA
CALVANI, M
NOBILI, L
[J]. ASTROPHYSICAL JOURNAL, 1980, 242 (02) : 772 - 788
[4] ON COLLIMATION OF RELATIVISTIC JETS FROM QUASARS
ABRAMOWICZ, MA
PIRAN, T
[J]. ASTROPHYSICAL JOURNAL, 1980, 241 (01) : L7 - L11
[5] BEAM MODELS FOR SS-433
BEGELMAN, MC
SARAZIN, CL
HATCHETT, SP
MCKEE, CF
ARONS, J
[J]. ASTROPHYSICAL JOURNAL, 1980, 238 (02) : 722 - 730
[6] HJELLMING RM, 1973, IAU S, V55, P98
[7] Jaroszynski M., 1980, Acta Astronomica, V30, P1
[8] KOZLOWSKI M, 1978, ASTRON ASTROPHYS, V63, P209
[9] GRAVITY POWER
LYNDENBELL, D
[J]. PHYSICA SCRIPTA, 1978, 17 (03): : 185 - 191
[10] PACZYNSKY B, 1980, ASTRON ASTROPHYS, V88, P23

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