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Article: The relationship between the radio and far-infrared emission in IRAS galaxies - VLA observations of a large well-defined sample at 1420 MHz

TitleThe relationship between the radio and far-infrared emission in IRAS galaxies - VLA observations of a large well-defined sample at 1420 MHz
Authors
Unger, SWWolstencroft, RDPedlar, ASavage, AClowes, RGLeggett, SKParker, QA
KeywordsFar Infrared Radiation
Galactic Radio Waves
Radio Astronomy
Star Formation
Astronomical Catalogs
Infrared Astronomy Satellite
Luminosity
Radiant Flux Density
Very Large Array (Vla)
Issue Date1989
PublisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/
Citation
Monthly Notices of the Royal Astronomical Society, 1989, v. 236, p. 425-446 How to Cite?
DOI: http://dx.doi.org/10.1093/mnras/236.3.425
AbstractAn examination of VLA observations at 1420 MHz of a well-defined sample of 156 IRAS galaxies reveals a strong correlation between the radio and far-infrared emission from IRAS galaxies. The flux density ratio is found to have a constant value of -4.82. The results suggest that the nonthermal radio emission is closely related to the current level of star formation, and that the star formation region in most IRAS galaxies is confined to the central few kpc of the galaxy.
Persistent Identifierhttp://hdl.handle.net/10722/211172
ISSN
0035-8711
2021 Impact Factor: 5.235
2020 SCImago Journal Rankings: 2.058
ISI Accession Number ID
WOS:A1989R919700011

 

DC FieldValueLanguage
dc.contributor.authorUnger, SW-
dc.contributor.authorWolstencroft, RD-
dc.contributor.authorPedlar, A-
dc.contributor.authorSavage, A-
dc.contributor.authorClowes, RG-
dc.contributor.authorLeggett, SK-
dc.contributor.authorParker, QA-
dc.date.accessioned2015-07-08T03:22:33Z-
dc.date.available2015-07-08T03:22:33Z-
dc.date.issued1989-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1989, v. 236, p. 425-446-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/211172-
dc.description.abstractAn examination of VLA observations at 1420 MHz of a well-defined sample of 156 IRAS galaxies reveals a strong correlation between the radio and far-infrared emission from IRAS galaxies. The flux density ratio is found to have a constant value of -4.82. The results suggest that the nonthermal radio emission is closely related to the current level of star formation, and that the star formation region in most IRAS galaxies is confined to the central few kpc of the galaxy.-
dc.languageeng-
dc.publisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectFar Infrared Radiation-
dc.subjectGalactic Radio Waves-
dc.subjectRadio Astronomy-
dc.subjectStar Formation-
dc.subjectAstronomical Catalogs-
dc.subjectInfrared Astronomy Satellite-
dc.subjectLuminosity-
dc.subjectRadiant Flux Density-
dc.subjectVery Large Array (Vla)-
dc.titleThe relationship between the radio and far-infrared emission in IRAS galaxies - VLA observations of a large well-defined sample at 1420 MHz-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.description.naturelink_to_OA_fulltext-
dc.identifier.doi10.1093/mnras/236.3.425-
dc.identifier.scopuseid_2-s2.0-4243702378-
dc.identifier.volume236-
dc.identifier.spage425-
dc.identifier.epage446-
dc.identifier.isiWOS:A1989R919700011-
dc.identifier.issnl0035-8711-

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