Stedy emission from recurrent transient pulsar 0535+26

Details Stedy emission from recurrent transient pulsar 0535+26 Stedy emission from recurrent transient pulsar 0535+26

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..158m&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 158-164 (1984).

Computer Science

X-Ray Sources, X-Ray Bursts, X-Ray Binaries, Pulsars

Scientific paper

A steady hard X-ray emission between 20-100 keV was observed from the 104 sec pulsar 0535+26 during the quiescent phase of transient activity. The present observations corespond to the binary phase of 0.7 taking 110d as the binary period. The observed flux was comparable to ~20 milli-crab and a power law spectrum with spectral index α~1.2 fits the data, and significantly differs from the observed spectrum during the outburst.

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