Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/34510
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dc.contributor.authorProtheroe, R.-
dc.contributor.authorMucke, A.-
dc.contributor.editorLaing, R.A.-
dc.contributor.editorBlundell, K.M.-
dc.date.issued2002-
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.113-116-
dc.identifier.isbn1583810900-
dc.identifier.issn1050-3390-
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.-
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.-
dc.description.statementofresponsibilityR.J. Protheroe, A. Mücke-
dc.language.isoen-
dc.publisherASP-
dc.relation.ispartofseriesAstronomical Society of the Pacific conference series ; v. 250-
dc.source.urihttp://arxiv.org/abs/astro-ph/0010625-
dc.subjectAstrophysics (astro-ph)-
dc.titleEstimating jet power in proton blazar models-
dc.typeConference paper-
dc.contributor.conferenceOxford Radio Galaxy Workshop (2000 : Oxford University)-
dc.publisher.placeUnited Kingdom-
pubs.publication-statusPublished-
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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