The FR II broad-line seyfert 1 galaxy: PKS J1037-2705
dc.contributor.author | Punsly, B. | |
dc.contributor.author | Clarke, T. | |
dc.contributor.author | Tingay, Steven | |
dc.contributor.author | Gutierrez, C. | |
dc.contributor.author | Rasmussen, J. | |
dc.contributor.author | Colbert, E. | |
dc.date.accessioned | 2017-01-30T15:06:31Z | |
dc.date.available | 2017-01-30T15:06:31Z | |
dc.date.created | 2009-05-14T02:17:14Z | |
dc.date.issued | 2008 | |
dc.identifier.citation | Punsly, Brian and Clarke, Tracy and Tingay, Steven and Gutierrez, Carlos and Rasmussen, Jesper and Colbert, E. 2008. The FR II broad-line seyfert 1 galaxy: PKS J1037-2705. The Astrophysical Journal. 687: pp. 162-172. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/43309 | |
dc.identifier.doi | 10.1086/591650 | |
dc.description.abstract |
In this article we demonstrate that PKS J1037-2705 has a weak accretion flow luminosity, well below the Seyfert 1/QSO dividing line, weak broad emission lines (BELs), and moderately powerful FR II extended radio emission. It is one of the few documented examples of a broad-line object in which the time-averaged jet kinetic luminosity, is larger than the total thermal luminosity (IR to X-ray) of the accretion flow, Lbol. The blazar nucleus dominates the optical and near-ultraviolet emission and is a strong source of hard X-rays. The strong blazar emission indicates that the relativistic radio jet is presently active. The implication is that even weakly accreting AGNs can create powerful jets. Kinetically dominated (Q>Lbol) broad-line objects provide important constraints on the relationship between the accretion flow and the jet production mechanism. | |
dc.publisher | The American Astronomical Society | |
dc.title | The FR II broad-line seyfert 1 galaxy: PKS J1037-2705 | |
dc.type | Journal Article | |
dcterms.source.volume | 687 | |
dcterms.source.startPage | 162 | |
dcterms.source.endPage | 172 | |
dcterms.source.issn | 0004637X | |
dcterms.source.title | The Astrophysical Journal | |
curtin.note |
This article appeared in The Astrophysical Journal and may be found at: | |
curtin.note |
Copyright © 2008. The American Astronomical Society. All rights reserved. | |
curtin.department | Department of Imaging and Applied Physics | |
curtin.accessStatus | Open access via publisher | |
curtin.faculty | Department of Medical Imaging and Applied Physics | |
curtin.faculty | School of Science | |
curtin.faculty | Faculty of Science and Engineering |