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Compact Radio Emission in 60 µm Peaker Galaxies

Published online by Cambridge University Press:  12 April 2016

C. A. Heisler ,
R. P. Norris ,
D. L. Jauncey ,
J. E. Reynolds  and
E. A. King
C. A. Heisler
Affiliation:
Mount Stromlo and Siding Spring Observatory, The Australian National University, ACT, 2611, Australia
R. P. Norris
Affiliation:
Australia Telescope National Facility, Epping, NSW, 2121, Australia
D. L. Jauncey
Affiliation:
Australia Telescope National Facility, Epping, NSW, 2121, Australia
J. E. Reynolds
Affiliation:
Australia Telescope National Facility, Epping, NSW, 2121, Australia
E. A. King
Affiliation:
Australia Telescope National Facility, Epping, NSW, 2121, Australia

Abstract

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We present radio interferometric observations of a well defined sample of IRAS galaxies with warm far-infrared colors — 60 µm Peakers (60PKs). The core radio power of 60PKs is intermediate to that of “normal” Seyfert 2 galaxies and radio ellipticals, and follows the same relationship with respect to total radio emission as low and high power radio galaxies. This is consistent with the suggestion that 60PKs represent nascent radio elliptical galaxies.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 211 - 212
Copyright
Copyright © Astronomical Society of the Pacific 1998

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