| dc.contributor.author | Hardcastle, M. J. | |
| dc.date.accessioned | 2019-01-22T14:45:01Z | |
| dc.date.available | 2019-01-22T14:45:01Z | |
| dc.date.issued | 2018-04-05 | |
| dc.identifier.citation | Hardcastle , M J 2018 , ' Interpreting radiative efficiency in radio-loud AGNs ' , Nature Astronomy , vol. 2 , no. 4 , pp. 273-274 . https://doi.org/10.1038/s41550-018-0424-1 | |
| dc.identifier.issn | 2397-3366 | |
| dc.identifier.other | ArXiv: http://arxiv.org/abs/1804.04043v1 | |
| dc.identifier.uri | http://hdl.handle.net/2299/21004 | |
| dc.description | Author submitted version of unrefereed Nature Astronomy comment. Version in journal format available at https://rdcu.be/KH6W | |
| dc.description.abstract | Radiative efficiency in radio-loud active galactic nuclei is governed by the accretion rate onto the central black hole rather than directly by the type of accreted matter; while it correlates with real differences in host galaxies and environments, it does not provide unambiguous information about particular objects. | en |
| dc.format.extent | 2 | |
| dc.format.extent | 281112 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Nature Astronomy | |
| dc.subject | Astronomy and Astrophysics | |
| dc.title | Interpreting radiative efficiency in radio-loud AGNs | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Non peer reviewed | |
| dc.date.embargoedUntil | 2018-11-05 | |
| dc.identifier.url | http://www.scopus.com/inward/record.url?scp=85045211405&partnerID=8YFLogxK | |
| rioxxterms.versionofrecord | 10.1038/s41550-018-0424-1 | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
