Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/34510
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dc.contributor.authorProtheroe, R.en
dc.contributor.authorMucke, A.en
dc.date.issued2002en
dc.identifier.citationParticles and fields in radio galaxies : proceedings of the Oxford Radio Galaxy Workshop held at Oxford University, Department of Astrophysics, Oxford, United Kingdom, 3-5 August, 2000 / Robert A. Laing and Katherine M. Blundell (eds.): pp.113-116en
dc.identifier.isbn1583810900en
dc.identifier.issn1050-3390en
dc.identifier.urihttp://hdl.handle.net/2440/34510-
dc.description© Copyright © 2002. Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. Submitted to Cornell University’s online archive www.arXiv.org in 2002 by Ray Protheroe. Post-print sourced from www.arxiv.org.en
dc.description.abstractWe discuss the various contributions to the jet luminosity in proton blazar models of active galactic nuclei and describe a method of estimating the jet luminosity from the observed spectral energy distribution (SED) and the fitted model parameters. We apply this to a synchrotron proton blazar (SPB) model for Markarian 501.en
dc.description.statementofresponsibilityR.J. Protheroe, A. Mückeen
dc.language.isoenen
dc.publisherASPen
dc.relation.ispartofseriesAstronomical Society of the Pacific conference series ; v. 250en
dc.source.urihttp://arxiv.org/abs/astro-ph/0010625en
dc.subjectAstrophysics (astro-ph)en
dc.titleEstimating jet power in proton blazar modelsen
dc.typeConference paperen
dc.identifier.rmid0020064664en
dc.contributor.conferenceOxford Radio Galaxy Workshop (2000 : Oxford University)en
dc.publisher.placeUnited Kingdomen
dc.identifier.pubid50171-
pubs.library.collectionChemistry and Physics publicationsen
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
Appears in Collections:Chemistry and Physics publications

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