EXOSAT observations of the 35d intensity variations of HER X-1

Details EXOSAT observations of the 35d intensity variations of HER X-1 EXOSAT observations of the 35d intensity variations of HER X-1

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xras.rept...16o&link_type=abstract

In its Contrib. of the X-Ray Astron. Group p 16-19 (SEE N85-20952 11-89)

Other

Binary Stars, Hercules Nova, Luminous Intensity, Pulsars, X Ray Sources, X Ray Spectra, Exosat Satellite, Light Curve, Periodic Variations

Scientific paper

Following the 4 to 7 cycle prlonged off state of Her X-1, the source was observed by EXOSAT through a normal 35d cycle. The observations started on 1 March 1984 and covered one full 35d cycle from one high on state to another at 4 day intervals. The medium energy flux (2 to 20 keV) in the argon counters varies by a factor of 50 during this cycle, as in the past. The low energy telescope data in the 0.04 to 2 keV range represents the first 35d cycle sampling of the soft X-rays. The observed light curve is similar to the medium energy light curve.

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