HELIOS 2-Vela-Ariel 5 gamma-ray burst source position

Details HELIOS 2-Vela-Ariel 5 gamma-ray burst source position HELIOS 2-Vela-Ariel 5 gamma-ray burst source position

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...229l..47c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 229, Apr. 15, 1979, p. L47-L51. Research supported by the Science Re

Astronomy and Astrophysics

Astronomy

24

Gamma Ray Astronomy, Radiation Sources, Satellite Observation, Ariel 5 Satellite, Helios 2, Vela Satellites

Scientific paper

The gamma-ray burst of January 28, 1976, one of 18 events thus far detected in interplanetary space with Helios 2, was also observed with the Vela 5A and 6A and the Ariel 5 satellites. A small source field is obtained from the intersection of the region derived from the observed time delays between Helios 2 and Vela 5A and 6A, with the source region independently found with the Ariel 5 X-ray detector. This area contains neither any steady X-ray source as scanned by HEAO 1 nor any previously cataloged X-ray, radio, or infrared sources, X-ray transients, quasars, Seyferts, globular clusters, flare stars, pulsars, white dwarfs, or high enery gamma-ray sources. The region is, however, within the source field of a gamma-ray transient observed in 1974 by Jacobson et al. (1978) which exhibited nuclear gamma-ray line structure.

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