Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ppas.book..171s&link_type=abstract
IN: Particle physics and astrophysics - Current viewpoints (A90-35283 15-90). Berlin and New York, Springer-Verlag, 1989, p. 171
Astronomy and Astrophysics
Astronomy
Black Holes (Astronomy), Gravitational Collapse, Neutron Stars, Stellar Mass, X Ray Binaries, Active Galactic Nuclei, Milky Way Galaxy, Radio Sources (Astronomy), Star Formation
Scientific paper
No unique characteristic has yet been conceived which would allow the unmistakable observational recognition of a black hole, partly due to the difficulty involved in distinguishing stellar black holes from weakly-magnetized neutron stars. Accordingly, all evidence for black holes rests on mass determinations of compact objects in X-ray binaries. Attention is presently given to three candidates: Cygnus X-1, LMC X-3, and A0620-00. The last of these, an X-ray nova, is judged to be the most likely candidate.
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