Time-Dependent Radiation Transfer and a Possible Explanation of the Interpulse in CP 0950

Details Time-Dependent Radiation Transfer and a Possible Explanation of the Interpulse in CP 0950 Time-Dependent Radiation Transfer and a Possible Explanation of the Interpulse in CP 0950

Sep 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..18...21d&link_type=abstract

Astrophysics and Space Science, Volume 18, Issue 1, pp.21-33

Astronomy and Astrophysics

Astrophysics

Scientific paper

The time-dependent equation of radiative transfer is solved exactly and in then-th Gaussian approximation. The atmosphere is plane-parallel and semi-infinite; isotropic scattering is assumed, but the boundary condition at τ=0 is arbitrary. The results are used to investigate a suggested mechanism for the origin of the secondary pulses in CP 0950; it is found that a binary system of neutron stars can indeed explain formation, time delay and intensity of the observed interpulse.

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