Soft gamma-ray bursts from the source B1900+14

Details Soft gamma-ray bursts from the source B1900+14 Soft gamma-ray bursts from the source B1900+14

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979sval....5..343m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Dec. 1979, p. 641-643.) Soviet Astronomy Letters, vol. 5, Nov.-Dec. 1979, p. 343, 34

Astronomy and Astrophysics

Astronomy

86

Bursts, Energy Spectra, Gamma Ray Astronomy, Pulsars, Spaceborne Astronomy, X Ray Sources, Gamma Rays, Satellite Observation, Stellar Mass Accretion, Thermonuclear Reactions, Time Dependence, Venera Satellites

Scientific paper

Three gamma-ray bursts from a source designated B1900+14 which have been recorded with a 1/64-sec resolution in the 50-150 keV energy window are discussed. For the three events, the rise time is no longer than 8 msec; the abrupt rise in intensity is then followed by a rapid decline. Altogether the bursts lasted 120, 190, and 50 msec. The energy of the source is roughly estimated at about 10 to the 39th erg, which could be produced by nonsteady accretion onto a compact star, or by thermonuclear flashes.

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