The high galactic latitude fast-transient X-ray source 3A 1431 - 409

Details The high galactic latitude fast-transient X-ray source 3A 1431 - 409 The high galactic latitude fast-transient X-ray source 3A 1431 - 409

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.201p..31m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 201, Nov. 1982, p. 31P-37P. Research supported by the Science and Engin

Astronomy and Astrophysics

Astronomy

8

Variable Stars, X Ray Sources, Ariel 5 Satellite, H Alpha Line, High Resolution, Light Curve, Stellar Color, Stellar Magnitude, Stellar Spectra

Scientific paper

X-ray observations of the fast-transient source 3A 1431 - 409 and optical observations of the RS CVn-like system 'V532 Cen star 1, which is proposed as a probable identification for the X-ray source, are presented. The physical parameters of the system are discussed and it is shown that, assuming the identification is correct, this is the most energetic X-ray event so far detected from an RS CVn-like system.

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