Abstract
PSR B0656+14s 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 St phase-resolved optical photometry is shown to constrain this characterisation.
| Original language | English (Ireland) |
|---|---|
| Title of host publication | Pulsar Astronomy - 2000 And Beyond: IAU Colloquium 177 |
| Place of Publication | Bonn, Germany |
| Publication status | Published - 1 Jan 2000 |
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