Herschel-ATLAS/GAMA: a difference between star formation rates in strong-line and weak-line radio galaxies

We have constructed a sample of radio-loud objects with optical spectroscopy from the Galaxy and Mass Assembly (GAMA) project over the Herschel Astrophysical Terahertz Large Area Survey (Herschel-ATLAS) Phase 1 fields. Classifying the radio sources in terms of their optical spectra, we find that str...

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Dettagli Bibliografici
Autori principali:	Hardcastle, M, Ching, J, Virdee, J, Jarvis, M, Croom, S, Sadler, E, Mauch, T, Smith, D, Stevens, J, Baes, M, Baldry, I, Brough, S, Cooray, A, Dariush, A, De Zotti, G, Driver, S, Dunne, L, Dye, S, Eales, S, Hopwood, R, Liske, J, Maddox, S, Michalowski, M, Rigby, E, Robotham, A
Natura:	Journal article
Lingua:	English
Pubblicazione:	2013

Herschel-ATLAS/GAMA: a difference between star formation rates in strong-line and weak-line radio galaxies

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