Accretion powered X-ray pulsars

Details Accretion powered X-ray pulsars Accretion powered X-ray pulsars

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8335957w&link_type=abstract

Unknown

Computer Science

Luminosity, Pulsars, X Ray Sources, Accretion Disks, Spectrum Analysis, X Ray Spectra

Scientific paper

A unified description of the properties of 14 X-ray pulsars is presented and compared with the current theoretical understanding of these systems. The sample extends over six orders of magnitude in luminosity, with the only trend in the phase averaged spectra being that the lower luminosity systems appear to have less abrupt high energy cutoffs. There is no correlation of luminosity with power law index, high energy cutoff energy or iron line EW. Detailed pulse phase spectroscopy is given for five systems.

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