Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ans..conf..112f&link_type=abstract
In Max-Planck Inst. Phys. and Astrophys. Accreting Neutron Stars p 112-116 (SEE N83-15179 05-88)
Astronomy and Astrophysics
Astrophysics
1
Pulsars, Pulse Rate, X Ray Sources, Energy Spectra, Spectrum Analysis, Time, Variability, X Ray Spectra
Scientific paper
The X-ray source A0535+26 is well established as a recurrent transient. During its activity it shows long period pulsations with a relevant and variable rate of decrease of the pulse period. On the basis of its peak luminosity and pulsation features, the source has been suggested as an accreting neutron star in a binary system. In September to October 1980 the source showed a very high level outburst. A flux level in the 1-12 keV energy range. The source was observed in the hard X-ray energy range on October 5th. Due to high signal from A0535+26 the observation resulted to be very effective to study its time variability and energy spectrum.
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