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PSR B0656+14: Combined Optical, X-ray & EUV Studies
Published online by Cambridge University Press: 12 April 2016
Abstract
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PSR B0656+14’s high energy emission is consistent with that of combined magnetospheric and thermal (surface & polar cap) emission. Uncertainties with the radio-derived distance and X-ray instrumentation sensitivities complicate a definitive thermal characterisation however. A re-analysis of combined ROSAT/EUVE archival data in conjunction with integrated & phase-resolved optical photometry is shown to constrain this characterisation.
- Type
- Part 4. Optical Observations
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 299 - 300
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
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