The wind and shock model for quasars - Confrontation with observations of 3C 273

Details The wind and shock model for quasars - Confrontation with observations of 3C 273 The wind and shock model for quasars - Confrontation with observations of 3C 273

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224...10c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. 10-16.

Astronomy and Astrophysics

Astrophysics

25

Astronomical Models, Astronomical Spectroscopy, Quasars, Stellar Winds, Infrared Radiation, Light Curve, Shock Waves, Synchrotron Radiation, X Ray Sources

Scientific paper

The wind and shock model for quasars is confronted to observations of 3C 273 obtained since late 1983. It is seen that the hypothesis of spherical symmetry used for simplicity in the original model has to be abandoned. Two physical mechanisms that could lead to physical conditions similar to those empirically derived from the model are proposed.

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