RELATIVISTIC EFFECTS IN SUPERLUMINAL JETS AND NEUTRON-STAR WINDS

被引:63
作者
ABRAMOWICZ, MA
ELLIS, GFR
LANZA, A
机构
[1] UNIV CHICAGO,DEPT ASTRON & ASTROPHYS,CHICAGO,IL 60637
[2] INT CTR THEORET PHYS,I-34100 TRIESTE,ITALY
[3] UNIV CAPE TOWN,DEPT APPL MATH,CAPE TOWN,SOUTH AFRICA
关键词
Galaxies: jets; Relativity; Stars: winds;
D O I
10.1086/169211
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We give a complete solution to the problem of radial motion of a test particle through the combined gravitational and radiation field of a spherical star. The star is assumed to radiate isotropically from each point of its surface. The radiative force acting on the particle is assumed not to depend on the frequency of radiation. There is no feedback from the particle motion to the background radiation field. All the effects of special and general relativity are included with no approximation.
引用
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页码:470 / 482
页数:13
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