MODEL FOR SS-433 - PRECESSING JETS IN AN ULTRA-CLOSE BINARY-SYSTEM

被引：28

作者：

MARTIN, PG ^{[1
]}

REES, MJ ^{[1
]}

机构：

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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1979年 / 189卷 / 01期

关键词：

Binary systems - Black hole mass - Gas jet - Gravitational radiation - Hole spin - Lense-thirring effect - Mass loss - Orbital angular momentum - Spectral feature - Spin-axis;

D O I：

10.1093/mnras/189.1.19P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The peculiar spectral features of SS433 have been attributed to gas jets with c/4, precessing with 160-day period. We propose a mechanism involving a spinning black hole (mass 4 yr. The mass loss from the dwarf is highly 'supercritical'; most of this matter escapes as a wind, and gives rise to the rest-system spectral features. © Royal Astronomical Society • Provided by the NASA Astrophysics Data System.

引用

页码：P19 / P22

页数：4

共 16 条

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[3] SS-433 - DOUBLE JET IN ACTION
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ANGEL, JRP
HEGE, EK
MARTIN, PG
BLAIR, WP
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[7] BIZARRE SPECTRUM OF SS-433
MARGON, B
FORD, HC
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ULRICH, RK
STONE, RPS
KLEMOLA, A
[J]. ASTROPHYSICAL JOURNAL, 1979, 230 (01) : L41 - L45
[8] MARTIN PG, 1979, IAU3358 CIRC
[9] MCGRAW J, 1979, IAU3363 CIRC
[10] MILGROM M, 1979, ASTRON ASTROPHYS, V76, pL3

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