GRO J0422+32
GRO J0422+32[1] is an X-ray nova and black hole candidate that was discovered by the BATSE instrument on the CGRO satellite on 5 August 1992.[2][3] During outburst, it was observed to be stronger than the Crab Nebula gamma-ray source out to photon energies of about 500 keV.[4]
The mass of the black hole in GRO J0422+32 falls in the range 3.66 to 4.97 solar masses.[5] This is the smallest yet found for any stellar black hole, and near the theoretical upper mass limit (~2.7 M☉) for a neutron star. Further analysis in 2012 calculated a mass of 2.1 M☉, which raises questions as to what the object actually is.[6]
Position (J2000) is RA 04 h 21 m 42.77 s +32 deg 54' 26.7".[7][8]
It is identified with an M1V variable star, V518 Per,[9] in the constellation Perseus, with magnitudes 13.5 in the B spectral band, and 13.2 in V.
References
- ↑ SIMBAD
- ↑ Harmon, A. et al. (1992) IAUC 5584
- ↑ Paciesas, W. et al. (1992), IAUC 5594
- ↑ Ling, J. C.; Wm; Wheaton, A. (2003). "BATSE Soft γ-Ray Observations of GROJ0422+32". Ap. J. 584: 399. arXiv:astro-ph/0210673. Bibcode:2003ApJ...584..399L. doi:10.1086/345602.
- ↑ http://adsabs.harvard.edu/abs/2003ApJ...599.1254G
- ↑ Kreidberg, Laura; Bailyn, Charles D.; Farr, Will M.; Kalogera, Vicky (2012). "Mass Measurements of Black Holes in X-ray Transients: is There a Mass Gap?" (PDF). The Astrophysical Journal 757 (36): 17pp. arXiv:1205.1805. Bibcode:2012ApJ...757...36K. doi:10.1088/0004-637x/757/1/36.
- ↑ McCroskey et al., IAUC 5594, 1992
- ↑ Castro-Tirado, A. J. et al. (1993), Astron.&Astrophys, "Discovery of the optical counterpart of the soft X-ray transient GRO J0422+32", vol. 276, no2, pp. L37-L40
- ↑ General Catalogue of Variable Stars, 3rd ed. (1971) Moscow
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