Gamma-ray bursts and radio pulsar glitches

Details Gamma-ray bursts and radio pulsar glitches Gamma-ray bursts and radio pulsar glitches

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...387..622h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 387, March 10, 1992, p. 622, 623. Research supported by Los Alamos National

Astronomy and Astrophysics

Astronomy

9

Gamma Ray Bursts, Pulsars, Satellite-Borne Instruments, Spaceborne Astronomy

Scientific paper

Upper limits to gamma-ray fluxes produced in conjunction with a radio pulsar glitch are presented. The glitch occurred on the Vela pulsar on December 24, 1988 and was the first to be observed as it occurred. Sensitive gamma-ray burst detectors aboard the Phobos 2 spacecraft were operating at this time, but recorded no significant burst at the time of the glitch. It is concluded that if a gamma-ray burst was generated in the energy range to which the Phobos detectors were sensitive, and if it was not beamed away from the spacecraft, the efficiency of glitch energy conversion into gamma-rays could not have exceeded 10 exp -4.

Affiliated with

Also associated with

No associations

Rating

Gamma-ray bursts and radio pulsar glitches does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gamma-ray bursts and radio pulsar glitches, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray bursts and radio pulsar glitches will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1215246