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1996A&AS..120C..69B - Astron. Astrophys., Suppl. Ser., 120C, 69-72 (1996/December-3)
ROSAT observations of gamma-ray pulsars: Vela, PSR 1706-44 and PSR 1951+32.
BECKER W. and TRUEMPER J.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): pulsars: individual (PSR 0833-45, PSR 1706-44, PSR 1951+32) - X-rays: stars - stars: neutron - gamma rays: observations
CDS comments: Misprint in the title and the keywords: read "PSR 1951+32" instead of "PSR 1951+31". Special Issue "3rd Compton Symposium"
Simbad objects: 14
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