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LOFAR/H-ATLAS: the low-frequency radio luminosity–star formation rate relation

Abstract:

Radio emission is a key indicator of star formation activity in galaxies, but the radio luminosity–star formation relation has to date been studied almost exclusively at frequencies of 1.4 GHz or above. At lower radio frequencies, the effects of thermal radio emission are greatly reduced, and so we would expect the radio emission observed to be completely dominated by synchrotron radiation from supernova-generated cosmic rays. As part of the LOFAR Surveys Key Science project, the Herschel-ATL...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/sty016

Authors


Gürkan, G More by this author
Hardcastle, MJ More by this author
Smith, DJB More by this author
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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
475
Issue:
3
Pages:
3010–3028
Publication date:
2018-01-09
Acceptance date:
2017-12-28
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:820591
URN:
uri:11e0cae9-ed0c-49f9-a421-9231c60d9a9f
UUID:
uuid:11e0cae9-ed0c-49f9-a421-9231c60d9a9f
Local pid:
pubs:820591

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