X-ray pulsars observed with hakucho and tenma

Details X-ray pulsars observed with hakucho and tenma X-ray pulsars observed with hakucho and tenma

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..131n&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 131-138 (1984).

Physics

4

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

Scientific paper

The pulse periods of eight pulsars Her X-1, Cen X-3, Vela X-1, A0535+26, GX301-2, 4U1626-67, 4U1538-52, and OA01657-415, have been measured with HAKUCHO and TENMA satellites between March 1979 and July 1983. Not only the wind-fed X-ray pulsas such as Vela X-1, GX301-2 and A0535-26, but also Her X-1 and Cen X-3, which are considered to be disk-fed pulsars, exhibit a remarkable change in the spin-up rate.

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