X-ray pulsar models. I - Angle-dependent cyclotron line formation and comptonization

Details X-ray pulsar models. I - Angle-dependent cyclotron line formation and comptonization X-ray pulsar models. I - Angle-dependent cyclotron line formation and comptonization

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...298..147m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 298, Nov. 1, 1985, p. 147-160.

Astronomy and Astrophysics

Astrophysics

93

Astronomical Models, Cyclotron Radiation, Line Spectra, Pulsars, Stellar Atmospheres, X Ray Binaries, Boundary Value Problems, Compton Effect, Finite Difference Theory, Radiative Transfer

Scientific paper

A multiangle, incoherent scattering formalism that yields pulse phase spectroscopic information is used to calculate spectra and cyclotron line shapes of static X-ray pulsar atmospheres with slab and column geometry. Comparisons with observations of integrated spectra and of phase-dependent cyclotron line properties indicates a better fit for the slab models. The illumination of inner or outer boundaries by external photon sources is allowed for, and the examples considered are an arbitrary input at the inner boundary.

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