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Radio-Excess IRAS Galaxies: Low Power CSS/GPS Sources?

Published online by Cambridge University Press:  05 March 2013

Catherine L. Drake ,
Peter J. McGregor ,
Geoffrey V. Bicknell  and
Michael A. Dopita
Catherine L. Drake
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia. [email protected], [email protected], [email protected], [email protected] Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia.
Peter J. McGregor
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia. [email protected], [email protected], [email protected], [email protected]
Geoffrey V. Bicknell
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia. [email protected], [email protected], [email protected], [email protected]
Michael A. Dopita
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia. [email protected], [email protected], [email protected], [email protected]
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Abstract

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Amongst our sample of radio-excess IRAS galaxies, we have identified compact steep spectrum radio sources that fall into the classes of CSS or GPS sources, but have not previously been identified as such. The sample includes objects that have radio powers as low as ˜1022 W Hz−1. We suggest that these are low-power analogues of CSS and GPS sources, with weaker radio jets. These may be precursors to FR I radio galaxies or may ‘fade’ into radio-quiet galaxies.

Keywords

galaxies: activeinfrared: galaxiesradio continuum: galaxies
Type
GPS/CSS Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 1 , 2003 , pp. 57 - 61
Copyright
Copyright © Astronomical Society of Australia 2003

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