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Supercritical Accretion and its Possible Relation to Quasars and Radio Sources

Published online by Cambridge University Press:  14 August 2015

David L. Meier*
Affiliation:
Jet Propulsion Laboratory, Pasadena, California

Extract

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This paper reviews some of the properties of supercritical accretion which make it a possible model for the quasar optical central source and for producing the jet in radio sources. Some of the problems with this scenario can be remedied with alternative, but related, models.

Type
Research Article
Copyright
Copyright © Reidel 1982 

References

Abramowicz, M. A. and Piran, T.: 1980, Astrophys. J. Letters, 241, p.L7.Google Scholar
Begelman, M. C. and Meier, D. L.: 1981, Astrophys. J., in press.Google Scholar
Meier, D. L.: 1981, Astrophys. J., in press.Google Scholar
Scott, J. S., Christiansen, W. A., Weymann, R. J. and Schiano, A.: 1981, in preparation.Google Scholar
Shakura, N. I. and Sunyaev, R. A.: 1973, Astron. Astrophys., 24, p.337 (SS).Google Scholar