e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey

Gigahertz-peaked spectrum (GPS) radio sources are thought to be young objects which later evolve into Fanaro-Riley type I (FR I) and FR II radio galaxies. We have used the Australia Telescope 20 GHz (AT20G) survey catalogue to select a uniform sample of GPS sources with spectral peaks above 5 GHz, w...

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Main Authors: Hancock, P., Tingay, Steven, Sadler, E., Phillips, C., Deller, A.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2009
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/5754
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author Hancock, P.
Tingay, Steven
Sadler, E.
Phillips, C.
Deller, A.
author_facet Hancock, P.
Tingay, Steven
Sadler, E.
Phillips, C.
Deller, A.
author_sort Hancock, P.
building Curtin Institutional Repository
collection Online Access
description Gigahertz-peaked spectrum (GPS) radio sources are thought to be young objects which later evolve into Fanaro-Riley type I (FR I) and FR II radio galaxies. We have used the Australia Telescope 20 GHz (AT20G) survey catalogue to select a uniform sample of GPS sources with spectral peaks above 5 GHz, which should represent the youngest members of this class. In this paper, we present e-VLBI observations of 10 such objects which are associated with nearby(z< 0.15) galaxies and so represent a new population of local, low-power GPS sources. Oure-VLBI observations were carried out at 4.8 GHz with the Australia Telescope Long Baseline Array (LBA) using a real-time software correlator. All 10 sources were detected, and wereunresolved on scales of ~100 mas, implying that they are typically less than 100 pc in linear size
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format Journal Article
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T06:08:34Z
publishDate 2009
publisher Wiley-Blackwell Publishing Ltd.
recordtype eprints
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spelling curtin-20.500.11937-57542017-09-13T16:02:57Z e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey Hancock, P. Tingay, Steven Sadler, E. Phillips, C. Deller, A. continuum galaxies radio active interferometers instrumentation evolution Gigahertz-peaked spectrum (GPS) radio sources are thought to be young objects which later evolve into Fanaro-Riley type I (FR I) and FR II radio galaxies. We have used the Australia Telescope 20 GHz (AT20G) survey catalogue to select a uniform sample of GPS sources with spectral peaks above 5 GHz, which should represent the youngest members of this class. In this paper, we present e-VLBI observations of 10 such objects which are associated with nearby(z< 0.15) galaxies and so represent a new population of local, low-power GPS sources. Oure-VLBI observations were carried out at 4.8 GHz with the Australia Telescope Long Baseline Array (LBA) using a real-time software correlator. All 10 sources were detected, and wereunresolved on scales of ~100 mas, implying that they are typically less than 100 pc in linear size 2009 Journal Article http://hdl.handle.net/20.500.11937/5754 10.1111/j.1365-2966.2009.15055.x Wiley-Blackwell Publishing Ltd. unknown
spellingShingle continuum
galaxies
radio
active
interferometers
instrumentation
evolution
Hancock, P.
Tingay, Steven
Sadler, E.
Phillips, C.
Deller, A.
e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey
title e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey
title_full e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey
title_fullStr e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey
title_full_unstemmed e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey
title_short e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey
title_sort e-vlbi observations of ghz-peaked spectrum radio sources in nearby galaxies from the at20g survey
topic continuum
galaxies
radio
active
interferometers
instrumentation
evolution
url http://hdl.handle.net/20.500.11937/5754