Group - GRO J0422+32

 


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    GRO J0422+32 is an X-ray nova and black hole candidate that was discovered by the BATSE instrument on the CGRO satellite on 5 August 1992. During outburst, it was observed to be stronger than the Crab Nebula gamma-ray source out to photon energies of about 500 keV. Position (J2000) is RA 04 h 21 m 42.77 s +32 deg 54' 26.7". It is identified with an M4.5V variable star, V518 Per, in the constellation Perseus, with magnitudes 13.5 in the B spectral band, and 13.2 in V. 



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