The case for a burst from 3U 0614+09

Details The case for a burst from 3U 0614+09 The case for a burst from 3U 0614+09

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.182..349s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 182, Feb. 1978, p. 349-353.

Astronomy and Astrophysics

Astronomy

44

Flare Stars, X Ray Astronomy, Ariel 5 Satellite, Binary Stars, Black Body Radiation, Bremsstrahlung, Light Curve, Oso-8, Stellar Models, X Ray Sources

Scientific paper

A single flare event with a rise time of about 7 s and a decay time of approximately 40 s was observed by the Goddard cosmic X-ray spectroscopy experiment on OSO-8 during observations of 3U 0614+09 in September 1975. The possibility is discussed that the source was 3U 0614+09, which has been compared with the low-mass binary Sco X-1. The spectra during the event could be fitted with blackbody (kT = 0.8-1.1 keV) or thermal bremsstrahlung (kT = 1.1-2.5 keV) models with absorption by cool material. In the blackbody model the source was of the order of 1 million cm in size.

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