Quasars at 25

Details Quasars at 25 Quasars at 25

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sci...234..155t&link_type=abstract

Science (ISSN 0036-8075), vol. 234, Oct. 10, 1986, p. 155-161.

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Black Holes (Astronomy), Quasars, Absorption Spectra, Dark Matter, Galactic Evolution, Radio Jets (Astronomy), Relativistic Velocity

Scientific paper

The characteristics of QSOs are analyzed. The determination of a distance scale for QSOs from absorption spectra in order to study the properties of QSOs is discussed. It is hypothesized that the energy sources for QSOs are black holes of 10 to the 6th-10 to the 11th solar masses; the conversion of this energy using three extractions mechanisms is examined. The formation of QSOs is described. Consideration is given to the Compton scattering problem, Doppler boosting, relativistic beaming, and the unified scheme for QSOs. The use of quasars and QSOs as probes for the location of redshift galaxies and clusters and dark matter, and the examination of QSO clustering is studied.

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