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

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dc.contributor.authorMcGregor, Peter
dc.contributor.authorBicknell, Geoffrey
dc.contributor.authorDopita, Michael
dc.contributor.authorDrake, Catherine
dc.coverage.spatialKerastari Greece
dc.date.accessioned2015-12-13T23:09:17Z
dc.date.available2015-12-13T23:09:17Z
dc.date.createdMay 29 2002
dc.date.issued2003
dc.date.updated2015-12-12T08:18:30Z
dc.description.abstractAmongst 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.
dc.identifier.urihttp://hdl.handle.net/1885/86929
dc.publisherCSIRO Publishing
dc.relation.ispartofseriesWorkshop on Compact Steep Spectrum and GHz-Peaked Spectrum Radio Sources 2002
dc.sourceThe Third Workshop on Compact Steep Spectrum and GHz-Peaked Spectrum Radio Sources
dc.subjectKeywords: Galaxies: active; Infrared: galaxies; Radio continuum: galaxies
dc.titleRadio-Excess IRAS Galaxies: Low Power CSS/GPS sources?
dc.typeConference paper
local.bibliographicCitation.lastpage61
local.bibliographicCitation.startpage57
local.contributor.affiliationMcGregor, Peter, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBicknell, Geoffrey, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDrake, Catherine, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidMcGregor, Peter, u8401248
local.contributor.authoruidBicknell, Geoffrey, u8000061
local.contributor.authoruidDopita, Michael, u7501303
local.contributor.authoruidDrake, Catherine, u9816101
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub15994
local.identifier.doi10.1071/AS02057
local.identifier.scopusID2-s2.0-18744388150
local.type.statusPublished Version

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