Abstract
We report upper limits to the 50 keV-10 MeV gamma-ray pulsations from PSR 1509-58 and PSR 0833-45 (Vela) made with the HEAO 3 gamma-ray spectrometer. The 2 σ upper limit to the 50-300 keV flux from PSR 1509-58 is 6.9 × 10-6 photons cm-2 s-1 keV-1. Combined with the best-fit X-ray spectrum, this limit suggests there is a break in the spectrum below ∼100 keV. This upper limit is not stringent enough, however, to distinguish between thermal and nonthermal models for the source of the X-ray emission. The 2 σ upper limit to the 3.2-10 MeV flux from PSR 0833-45 is 4.9 × 10-8 photons cm-2 s-1 keV-1.
Original language | English (US) |
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Pages (from-to) | 485-489 |
Number of pages | 5 |
Journal | Astrophysical Journal |
Volume | 369 |
Issue number | 2 |
DOIs | |
State | Published - Mar 10 1991 |
Keywords
- Gamma rays: bursts
- Pulsars
- Stars: individual (PSR 1509-58, PSR 0833-45)
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science