ROSAT observations of gamma-ray pulsars: Vela, PSR 1706-44 and PSR 1951+32.

Details ROSAT observations of gamma-ray pulsars: Vela, PSR 1706-44 and PSR 1951+32. ROSAT observations of gamma-ray pulsars: Vela, PSR 1706-44 and PSR 1951+32.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..120c..69b&link_type=abstract

Astronomy and Astrophysics Supplement, v.120, p.69-72

Astronomy and Astrophysics

Astrophysics

13

Pulsars: Individual (Psr 0833-45, Psr 1706-44, Psr 1951+32), X-Rays: Stars, Stars: Neutron, Gamma Rays: Observations

Scientific paper

The number of rotation-powered pulsars detected in both the X- and γ-ray wavebands has increased to seven. While the γ-ray emission of all these pulsars is found to be strongly pulsed at the rotational period of the radio pulsar no pulsed X-ray emission was detectable in the ROSAT data available from PSR 1706-44. For the X-ray pulses of PSR 1951+32 only a ~2σ signal was claimed. In this paper we show that the absence of pulsed X-ray emission from these two pulsars can be understood in terms of a Vela-like X-ray emission characteristics.

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