Detection of Soft X-Ray Emission from PSR 0833-45
Abstract
An observation of the Vela pulsar in the energy range 0.7-1.5 keV is presented. A comparison of the flux in this band with the spectrum of the source 3U 0833-45 for the 2-10 keV band suggests a low-energy turnover in the spectrum. The measurement is compared with other observations, and possible explanations of the turnover are discussed. Subject headings: pulsars - X-ray sources
- Publication:
-
The Astrophysical Journal
- Pub Date:
- May 1974
- DOI:
- 10.1086/181490
- Bibcode:
- 1974ApJ...190L...9C