The high-energy properties of X ray pulsars

Details The high-energy properties of X ray pulsars The high-energy properties of X ray pulsars

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296...57f&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 57-69 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

10

Pulsar Magnetospheres, Pulsars, Spectral Energy Distribution, X Ray Binaries, Energy Spectra, Line Spectra, Spectrum Analysis, Stellar Magnetic Fields, Stellar Spectra

Scientific paper

The properties of X-ray pulsars in hard X-rays are reviewed. The presence in the X-ray spectra of lines, probably due to the presence of superstrong magnetic fields, is revealed. The high energy band X-ray pulsars have much simpler pulse profiles and the modulation index shows a general trend to increase. The spectra show great variations in hardness from source to source. The analysis suggests that the harder sources are those with the most intense magnetic fields. The results obtained from pulse-phase spectroscopy and from temporal analysis of aperiodic variations in the flux at high energies are reviewed.

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