Remnant radio galaxies discovered in a multi-frequency survey

Remnant radio galaxies discovered in a multi-frequency survey

The remnant phase of a radio galaxy begins when the jets launched from an active galactic nucleus are switched off. To study the fraction of radio galaxies in a remnant phase, we take advantage of a deg subregion of the GAMA 23 field which comprises of surveys covering the frequency range 0.1-9 GHz....

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Bibliographic Details
Main Authors: Quici, B., Hurley-Walker, Natasha, Seymour, Nick, Turner, Ross, Shabala, S.S., Huynh, M., Andernach, H., Kapińska, A.D., Collier, J.D., Johnston-Hollitt, Melanie, White, S.V., Prandoni, I., Galvin, Tim, Franzen, Thomas, Ishwara-Chandra, C.H., Bellstedt, S., Tingay, Steven, Gaensler, B.M., O'Brien, A., Rogers, J., Chow, K., Driver, S., Robotham, A.
Format: Journal Article
Language:English
Published: CAMBRIDGE UNIV PRESS 2021
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
galaxies: active
methods: statistical
radio continuum: galaxies
ARRAY
EVOLUTION
LUMINOSITY
ENERGETICS
EMISSION
CLUSTERS
NUCLEI
MODELS
LOBES
AGN
astro-ph.GA
Online Access:http://purl.org/au-research/grants/arc/FT190100231
http://hdl.handle.net/20.500.11937/91778

Internet

http://purl.org/au-research/grants/arc/FT190100231
http://hdl.handle.net/20.500.11937/91778

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