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The Morphology of Sérsic-Pastoriza Galaxies

Published online by Cambridge University Press:  12 April 2016

G.J. Yates ,
A. Pedlar ,
D.J. Saikia ,
S.W. Unger  and
D.J. Axon
G.J. Yates
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, England
A. Pedlar
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, England
D.J. Saikia
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, England GMRT project, Tata Institute of Fundamental Research, Poona University Campus, Ganeshkhind, Pune 411007, India
S.W. Unger
Affiliation:
Royal Greenwich Observatory, Herstmonceux Castle, Hailsham, East Sussex, BN27 1RP, England
D.J. Axon
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, England

Abstract

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In this paper we present the preliminary results of our radio-continuum and neutral hydrogen observations of Sérsic-Pastoriza (S-P) galaxies. We show that the central regions contain a population of compact features thought to be young supernova remnants (SNRs) and discuss the overall morphology of the nuclei.

Type
III. Observations of Related Objects
Information
International Astronomical Union Colloquium , Volume 124: Paired and Interacting Galaxies , 1990 , pp. 245 - 249
Copyright
Copyright © NASA 1990

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