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dc.contributor.authorProtheroe, R.en
dc.contributor.authorMucke, A.en
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.description© Copyright © 2002. Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. Submitted to Cornell University’s online archive in 2002 by Ray Protheroe. Post-print sourced from
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.relation.ispartofseriesAstronomical Society of the Pacific conference series ; v. 250en
dc.subjectAstrophysics (astro-ph)en
dc.titleEstimating jet power in proton blazar modelsen
dc.typeConference paperen
dc.contributor.conferenceOxford Radio Galaxy Workshop (2000 : Oxford University)en
dc.publisher.placeUnited Kingdomen
pubs.library.collectionChemistry and Physics publicationsen
Appears in Collections:Chemistry and Physics publications

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