H0547-14 - X-ray flux from a weak gamma-ray burst?

Details H0547-14 - X-ray flux from a weak gamma-ray burst? H0547-14 - X-ray flux from a weak gamma-ray burst?

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269..779a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 269, June 15, 1983, p. 779-790.

Astronomy and Astrophysics

Astrophysics

8

Gamma Ray Bursts, M Stars, Stellar Flares, X Ray Sources, Bremsstrahlung, Dwarf Stars, Flare Stars, Heao 1, Late Stars, Light Curve

Scientific paper

Data concerning a fast X ray transient observed by the HEAO 1 on March 17, 1978 are discussed. The object, labeled H0547-14, was located in Lepus, with galactic coordinates 219.37 deg longitude, b = -20.12 deg in the anticenter direction. A 10 sec scan of the transient was obtained with proportional counter detectors. An X ray luminosity of more than 5.1 x 10 to the 31st ergs/sec was measured as a lower limit, with the decay taking 17 min. A lower limit to the flare was set at 30 sec. The flux intensity resided in the range 4.4/1 billion-4/100 million erg/sq cm per sec, with a rise time of a factor of 10 in about 5 sec. Possible characterizations of the object, as either a gamma ray burst or as an M dwarf star, are discussed.

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