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Conference Paper: Radio and optical studies of a complete sample of IRAS galaxies

TitleRadio and optical studies of a complete sample of IRAS galaxies
Authors
Wolstencrof, RDUnger, SWPedlart, AHeasley, JNParker, QAMenzies, JWSavage, AMacGillivray, HTLeggett, SKGang, WClowes, RG
Issue Date1-Jul-1988
PublisherSpringer Verlag
AbstractRadio maps, spectra and CCD images have been obtained for almost all the 158 objects in a complete sample of IRAS galaxies. The linear relation between radio and far-infrared luminosity is valid over the complete luminosity range (up to LIR = 1.8 x 1012LΘ, Ho= 75 km s−1Mpc−1). The majority of the 10 most luminous galaxies show evidence of tidal disruption and have companion galaxies at projected separations which range between 6 and 138 kpc. The second most luminous galaxy, IRAS 00275-2859, is a quasar with a spectrum reminiscent of a broad line absorption quasar and with a band of absorption running across the object: its infrared to radio luminosity ratio is identical to that of the typical IRAS galaxy.
Persistent Identifierhttp://hdl.handle.net/10722/342812

 

DC FieldValueLanguage
dc.contributor.authorWolstencrof, RD-
dc.contributor.authorUnger, SW-
dc.contributor.authorPedlart, A-
dc.contributor.authorHeasley, JN-
dc.contributor.authorParker, QA-
dc.contributor.authorMenzies, JW-
dc.contributor.authorSavage, A-
dc.contributor.authorMacGillivray, HT-
dc.contributor.authorLeggett, SK-
dc.contributor.authorGang, W-
dc.contributor.authorClowes, RG-
dc.date.accessioned2024-05-02T03:06:02Z-
dc.date.available2024-05-02T03:06:02Z-
dc.date.issued1988-07-01-
dc.identifier.urihttp://hdl.handle.net/10722/342812-
dc.description.abstractRadio maps, spectra and CCD images have been obtained for almost all the 158 objects in a complete sample of IRAS galaxies. The linear relation between radio and far-infrared luminosity is valid over the complete luminosity range (up to LIR = 1.8 x 1012LΘ, Ho= 75 km s−1Mpc−1). The majority of the 10 most luminous galaxies show evidence of tidal disruption and have companion galaxies at projected separations which range between 6 and 138 kpc. The second most luminous galaxy, IRAS 00275-2859, is a quasar with a spectrum reminiscent of a broad line absorption quasar and with a band of absorption running across the object: its infrared to radio luminosity ratio is identical to that of the typical IRAS galaxy.-
dc.languageeng-
dc.publisherSpringer Verlag-
dc.relation.ispartofThe Third IRAS Conference: Comets to Cosmology (06/07/1987-10/07/1987)-
dc.titleRadio and optical studies of a complete sample of IRAS galaxies-
dc.typeConference_Paper-
dc.identifier.doi10.1007/BFb0118810-
dc.identifier.scopuseid_2-s2.0-84946043153-
dc.identifier.volume297-
dc.identifier.spage202-
dc.identifier.epage205-

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