Published January 1990 | Version v1
Journal article

Observation of the Vela pulsar, PSR 0833-45, at 0.2-6.0 MeV with the FIGARO II experiment

  • 1. CEA, Service d'Astrophysique, Gif-sur-Yvette (France)
  • 2. Palermo Universita (Italy)
  • 3. CNR, Istituto di Fisica Cosmica con Applicazioni all'Informatica, Palermo (Italy)

Description

Results are reported of a 7.75 hr observation of PSR 0833-45 in Vela with FIGARO II (French Italian GAmma Ray Observatory) performed during a balloon flight on November 25, 1988. Two-sigma upper limits for the pulsar flux are given in the gamma-ray energy range 0.2-6.0 MeV. The values are significantly lower than the measured flux obtained by the Riverside experiment as reported by Tumay Tumer et al. in 1984, 31 days after a large glitch in the pulsar period. The FIGARO data also show a departure from the extrapolatian below 50 MeV of the time-averaged flux measured by the COS B satellite, suggesting the existence of a break in the quiescent energy spectrum for values at or obove 5-10 MeV. 7 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
349
Series
Astrophys. J.
Journal Page Range
L21-L24
ISSN
0004-637X
CODEN
ASJOA