Relativistic effects in superluminal jets and neutron star winds

Details Relativistic effects in superluminal jets and neutron star winds Relativistic effects in superluminal jets and neutron star winds

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...361..470a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 361, Oct. 1, 1990, p. 470-482. Research supported by the Ministero dell'Uni

Astronomy and Astrophysics

Astronomy

25

Neutron Stars, Particle Motion, Relativistic Effects, Stellar Winds, Eddington Approximation, Equations Of Motion, Lorentz Transformations, Radio Jets (Astronomy)

Scientific paper

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.

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