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

    Access Status
    Open access via publisher
    Authors
    Hancock, P.
    Tingay, Steven
    Sadler, E.
    Phillips, C.
    Deller, A.
    Date
    2009
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Hancock, Paul and Tingay, Steven and Sadler, E and Phillips, C and Deller, A. 2009. e-VLBI observations of GHz-peaked spectrum radio sources in nearby galaxies from the AT20G survey. Monthly Notices of the Royal Astronomical Society. 397 (4): pp. 2030-2036.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    DOI
    10.1111/j.1365-2966.2009.15055.x
    ISSN
    0035-8711
    Faculty
    Faculty of Science and Engineering
    Curtin Institute of Radio Astronomy
    URI
    http://hdl.handle.net/20.500.11937/5754
    Collection
    • Curtin Research Publications
    Abstract

    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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