The Milliarcsecond Structure of Radio Galaxies and Quasars-Reference-Cited by-同舟云学术

The Milliarcsecond Structure of Radio Galaxies and Quasars

Published:1982 Issue: Volume:97 Page:279-288
ISSN:0074-1809
Container-title:Symposium - International Astronomical Union
language:en
Short-container-title:Symp. - Int. Astron. Union

Author:

Readhead A.C.S.,Pearson T. J.

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.

Publisher

Cambridge University Press (CUP)

Reference36 articles.

1. Cotton W.D. , Geldzahler B.J. , and Shapiro I.I. : 1982, this volume, pp. 301–303.

2. VLBI observations of compact radio sources at 609 megahertz

3. Superluminal expansion of quasar 3C273

4. Milliarcsecond structure of 0428+205, 1518+047, and 2050+364 at 1.67 GHz

5. Mutel R.L. and Philips R.B. : 1982, this volume, p. 385.

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