Published 1982 | Version Published
Book Section - Chapter Open

The Milliarcsecond Structure of Radio Galaxies and Quasars

  • 1. ROR icon California Institute of Technology

Contributors

Abstract

Hybrid maps of the nuclei of radio galaxies and quasars show a variety of morphologies. Among compact sources, two structures are common: an asymmetric, "core-jet" morphology (eg, 3C 273), and an "equal double" morphology with two separated, similar components (eg, CTD 93). The nuclei of extended, double radio galaxies generally have a core-jet morphology with the jet directed toward one of the outer components.

Additional Information

© 1982 by the IAU. We thank our colleagues who kindly informed us of their results before publication, especially R.B. Phillips, R.L. Mutel, and S.C. Unwin, who provided several of the figures. VLBI at OVRO is supported by the NSF (AST 79-13249).

Attached Files

Published - milliarcsecond_structure_of_radio_galaxies_and_quasars.pdf

Files

milliarcsecond_structure_of_radio_galaxies_and_quasars.pdf

Files (962.3 kB)

Name Size
md5:f95a4ee45f0c9d0ea1044e5344000116
962.3 kB Preview Download

Additional details

Identifiers

Eprint ID
91430
Resolver ID
CaltechAUTHORS:20181204-104127778

Funding

NSF
AST 79-13249

Dates

Created
2018-12-04
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Series Name
IAU Symposium Proceedings Series
Series Volume or Issue Number
97