Optical Pre-Nova Identification for the X-Ray Nova GRO J0422+32 (Nova Persei, 1992)

Details Optical Pre-Nova Identification for the X-Ray Nova GRO J0422+32 (Nova Persei, 1992) Optical Pre-Nova Identification for the X-Ray Nova GRO J0422+32 (Nova Persei, 1992)

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...74..489k&link_type=abstract

Space Science Reviews, Volume 74, Issue 3-4, pp. 489-492

Physics

X-Ray Nova, Optical Counterpart, Black Hole Candidate

Scientific paper

The X-ray Nova GRO J0422+32 in its low brightness has been identified with a B˜ 21 m , R˜20 m star on Palomar Sky Survey glass copies. The scans obtained with an automatical microdensitometer along with our special PC program were used. The resulting outburst amplitude 8 m is one of similarity features for the class of the low mass X-ray Novae, black hole candidates.

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