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ASCA X-Ray Observations of the Vela Pulsar Jet

Published online by Cambridge University Press:  12 April 2016

Hakki Ögelman  and
Craig Markwardt
Hakki Ögelman
Affiliation:
University of Wisconsin, Madison
Craig Markwardt
Affiliation:
University of Wisconsin, Madison

Abstract

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An X-ray jet-like outflow, beginning at the Vela pulsar and extending about seven parsecs along the pulsar spin axis direction has recently been discovered (Markwardt & Ögelman 1995). We present data obtained by the X-ray ASCA satellite which confirms the enhanced X-ray emission at the jet head and discuss the allowable spectral models. The jet parameters are updated according to the combined ROSAT and ASCA results.

Type
Part 5 High Energy Phenomena
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 347 - 350
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Raymond, J.C. & Smith, B.W. 1977, ApJS, 35, 419.Google Scholar
Markwardt, C.B. & Ögelman, H. 1995, Nature, 375, 40.Google Scholar