Relativistic effects in superluminal jets and neutron star winds
Relativistic effects in superluminal jets and neutron star winds
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DOI：
10.1086/169211
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发表时间：
1990-10
期刊：
影响因子：
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通讯作者：
M. Abramowicz;G. Ellis;A. Lanza
中科院分区：
文献类型：
--
作者：
M. Abramowicz;G. Ellis;A. Lanza
A complete solution is given for 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. 29 refs.
