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1887
3561870
Accretion mode versus radio morphology in the LOFAR Deep Fields
Author(s):
Mingo, B.; Croston, J.H.; Best, P.N.; Duncan, K.J.; Hardcastle, M.J.; Kondapally, R.; Prandoni, I.; Sabater, J.; Shimwell, T.W.; Williams, W.L. (
0000-0001-7315-1596
); Baldi, R.D.; Bonato, M.; Bondi, M.; Dabhade, P.; Gürkan, G.; Ineson, J.; Magliocchetti, M.; Miley, G.; Pierce, J.C.S.; Röttgering, H.J.A.
Published
2022
Publication type
Article / Letter to editor
black hole physics galaxies
active
galaxies
jets
radio continuum galaxies
Astrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 511, no. 3, p. 3250-3271
hdl
1887/3561870
doi
10.1093/mnras/stac140
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.3250M
Persistent identifier url
https://hdl.handle.net/1887/3561870
Documents
01 - MNRAS_511_2022_3250
version: Publisher's Version
Full text at Publisher's site
Open Access