LOFAR/H-ATLAS: the low-frequency radio luminosity–star formation rate relation
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...
| Principais autores: | , , , , , , , , , , , , , |
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| Formato: | Journal article |
| Publicado em: |
Oxford University Press
2018
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