Observational status of black holes

Details Observational status of black holes Observational status of black holes

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979rspsa.368...27r&link_type=abstract

Royal Society (London), Proceedings, Series A - Mathematical and Physical Sciences, vol. 368, no. 1732, Oct. 17, 1979, p. 27-32.

Astronomy and Astrophysics

Astrophysics

2

Astrophysics, Black Holes (Astronomy), Galactic Nuclei, Gamma Rays, Globular Clusters, Gravitational Effects, Quasars, Radio Emission, Stellar Evolution, X Ray Sources

Scientific paper

Means of observing black holes are discussed. Consideration is given to the expected characteristics of possible indicators of solar-mass black holes in binary systems, massive black holes in globular clusters, massive black holes in galactic nuclei and quasars, intergalactic black holes, and miniholes, including characteristic X-ray emission, gravitational effects on neighboring stars, radio emission, gravitational lens images, cosmological effects and gamma-ray bursts. It is concluded that although there are strong reasons for suspecting that some astronomical systems contain black holes, their existence has not yet been confirmed.

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