Gamma-ray burst variability above 4 MeV

Details Gamma-ray burst variability above 4 MeV Gamma-ray burst variability above 4 MeV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1...51s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 51-54 (SEE N85-33902 22-93)

Astronomy and Astrophysics

Astronomy

Gamma Ray Bursts, Variations, X Rays, Energy Bands, Gamma Ray Spectrometers, Heao 3, Histories, Solar Maximum Mission, Spectra, Tables (Data), Time

Scientific paper

The relationship between the hard X-ray and gamma ray emissions during four bursts using the anti-coincidence shields of the High Energy Astronomy Observatory 3 (HEAO 3) Gamma Ray Spectrometer is explored. Recent observations of gamma ray bursts by the Solar Maximum Mission Gamma Ray Spectrometer (GRS) have shown that high energy emission above 1 MeV is a common and energetically important feature (Matz et al. 1985). Time histories of four gamma ray bursts in 3 energy bands ( keV, around 511 keV, and 4 MeV) with 10.24 a resolution show that the 4 MeV flux is only weakly coupled to the spectrum below approximately 600 keV.

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