SIMBAD references

2000ApJ...536..948S - Astrophys. J., 536, 948-953 (2000/June-3)

ROSAT observations of the Vela pulsar.

SEWARD F.D., ALPAR M.A., FLANAGAN C., KIZILOGLU U., MARKWARDT C., McCULLOCH P. and OEGELMAN H.

Abstract (from CDS):

The ROSAT HRI was used to monitor X-ray emission from the Vela pulsar. Six observations span 2.5 yr and three glitches. The summed data yield a determination of the pulse shape, and X-ray emission from the pulsar is found to be 12% pulsed with one broad and two narrow peaks. One observation occurred 15 days after a large glitch. No change in pulse structure was observed, and any change in X-ray luminosity, if present, was less than 3%. Implications for neutron star structure are discussed.

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Journal keyword(s): Stars: Pulsars: Individual: Name: Vela pulsar - Stars: Neutron - X-Rays: Stars

Simbad objects: 6

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