Pulse phase spectroscopy of HER X-1 with EXOSAT

Details Pulse phase spectroscopy of HER X-1 with EXOSAT Pulse phase spectroscopy of HER X-1 with EXOSAT

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xras.rept...20k&link_type=abstract

In its Contrib. of the X-Ray Astron. Group p 20-23 (SEE N85-20952 11-89)

Astronomy and Astrophysics

Astronomy

Binary Stars, Hercules Nova, Pulsars, X Ray Sources, X Ray Spectroscopy, Accretion Disks, Exosat Satellite, Stellar Coronas, Stellar Spectra

Scientific paper

During March/April 1984 Her X-1 was observed in a series of 10 pointings spread approximately evenly through a 35 day cycle. Pulse profiles and source spectra obtained during the on and short on state were analyzed. It is suggested that the interpulse of the 1.24 sec variation is caused by a reflection of the primary beam from the inner edge of the accretion disk or a disk corona.

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