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Cores in Extended Quasars

Published online by Cambridge University Press:  04 August 2017

P. D. Barthel ,
G. K. Miley ,
R. T. Schilizzi ,
E. Preuss  and
T. J. Cornwell
P. D. Barthel
Affiliation:
Leiden Observatory, Leiden, The Netherlands
G. K. Miley
Affiliation:
Leiden Observatory, Leiden, The Netherlands
R. T. Schilizzi
Affiliation:
NFRA, Dwingeloo, The Netherlands
E. Preuss
Affiliation:
MPIfR, Bonn, FRG
T. J. Cornwell
Affiliation:
NRAO, Socorro, USA

Extract

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The Nuclear Radio cores of several nearby extended radio galaxies (e.g. M87, 3C236) consist not only of optically thick (< 1 pc) components, but also of emission on somewhat larger scale. As extended radio sources associated with quasars have on average stronger and more luminous radio cores (see e.g. Miley, 1980, Ann. Rev. Astron. Astrophys. 18, 165), we have started a project to study the properties of these quasar cores.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 110: VLBI and Compact Radio Sources , 1984 , pp. 39 - 40
Copyright
Copyright © Reidel 1984