Gamma-ray bursts observed from the HINOTORI satellite

Details Gamma-ray bursts observed from the HINOTORI satellite Gamma-ray bursts observed from the HINOTORI satellite

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.105..379y&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 105, no. 2, Oct. 1984, p. 379-392.

Astronomy and Astrophysics

Astrophysics

2

Energy Spectra, Gamma Ray Bursts, Red Shift, Satellite Observation, Satellite-Borne Instruments, Gamma Ray Spectrometers, X Ray Spectroscopy

Scientific paper

During February, 1981 and June, 1982, the gamma-ray and the hard X-ray spectrometers on the Hinotori satellite observed four gamma-ray bursts on 28 February and 21 July, 1981 and 26 February and 13 March, 1982. These gamma-ray bursts were simultaneously observed by other satellites. The time histories and energy spectra are shown for these gamma-ray bursts, and the burst sizes (erg/sq cm) are estimated. Two possible source locations for the burst of 21 July, 1981 are roughly determined from arrival time delays between two pairs of satellites, PVO-Hinotori and ISEE-3-Hinotori. The weak gamma-ray line peak structure around 1.8 MeV was observed for the burst of 13 March, 1982. The line could be interpreted in terms of gravitationally redshifted neutron capture line at 2.22 MeV.

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