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dc.contributor.authorHoeppe, G.
dc.contributor.authorBrinks, E.
dc.contributor.authorKlein, U.
dc.contributor.authorGiovanardi, C.
dc.contributor.authorAltschuler, D.R.
dc.contributor.authorPrice, R.M.
dc.contributor.authorDeeg, H-J.
dc.date.accessioned2009-01-09T14:38:27Z
dc.date.available2009-01-09T14:38:27Z
dc.date.issued1994
dc.identifier.citationHoeppe , G , Brinks , E , Klein , U , Giovanardi , C , Altschuler , D R , Price , R M & Deeg , H-J 1994 , ' Radio continuum and far-infrared observations of low surface brightness galaxies ' , Astronomical Journal , vol. 108 , no. 2 , pp. 446-455 . https://doi.org/10.1086/117082
dc.identifier.issn1538-3881
dc.identifier.otherPURE: 150151
dc.identifier.otherPURE UUID: 81e25efe-5d4f-4ba1-8920-9ba078bbb6ba
dc.identifier.otherdspace: 2299/2784
dc.identifier.otherScopus: 0009735926
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407943
dc.identifier.urihttp://hdl.handle.net/2299/2784
dc.descriptionOriginal article can be found at: http://adsabs.harvard.edu/ Copyright American Astronomical Society DOI: 10.1086/117082 [Full text of this article is not available in the UHRA]
dc.description.abstractWe present Very Large Array (VLA) radio continuum and Infrared Astronomy Satellite (IRAS) far-infrared (FIR) observations of 16 low luminosity galaxies of mostly low surface brightness. All galaxies had previously claimed single dish radio continuum detections. However, at the frequencies of our observations (1.49 and 8.48 GHz), we find significant radio emission for two objects only. We show that the other previously claimed detections are due to confusion with physically unrelated background sources. This implies a low radio continuum detection rate for these galaxies. Re-reduced IRAS scans yield significant far-infrared flux densities in at least one IRAS band for 6 of the 16 galaxies. These, together with the FIR and radio continuum upper limits, are consistent with the well established radio/FIR relation, where most of our galaxies populate the low-luminosity end. From the radio continuum and FIR flux densities and their upper limits we estimate the current star formation rates and demonstrate that the galaxies are currently passive in forming stars, in agreement with previous optical investigations. There is an indication that the galaxies were forming stars more intensively averaged over their lifetime than they are presently.en
dc.language.isoeng
dc.relation.ispartofAstronomical Journal
dc.titleRadio continuum and far-infrared observations of low surface brightness galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1994
rioxxterms.versionofrecordhttps://doi.org/10.1086/117082
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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