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The Evolution of Shocks in Blazar Jets

Bicknell, Geoffrey; Wagner, Stefan J

Description

We consider the shock structures that can arise in blazar jets as a consequence of variations in the jet flow velocity. There are two possible cases: (1) a double shock system consisting of both a forward and reverse shock, and (2) a single shock (either

dc.contributor.authorBicknell, Geoffrey
dc.contributor.authorWagner, Stefan J
dc.date.accessioned2015-12-13T23:20:39Z
dc.date.available2015-12-13T23:20:39Z
dc.identifier.issn1323-3580
dc.identifier.urihttp://hdl.handle.net/1885/90802
dc.description.abstractWe consider the shock structures that can arise in blazar jets as a consequence of variations in the jet flow velocity. There are two possible cases: (1) a double shock system consisting of both a forward and reverse shock, and (2) a single shock (either
dc.publisherCSLI Publications
dc.sourcePublications of the Astronomical Society of Australia
dc.subjectKeywords: Acceleration of particles; BL Lacertae objects: general; BL Lacertae objects: individual (Mkn 501); Gamma rays: theory
dc.titleThe Evolution of Shocks in Blazar Jets
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume19
dc.date.issued2002
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub21267
local.type.statusPublished Version
local.contributor.affiliationBicknell, Geoffrey, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWagner, Stefan J, Ruprecht Karls University of Heidelberg
local.bibliographicCitation.startpage129
local.bibliographicCitation.lastpage137
local.identifier.doi10.1071/AS02009
dc.date.updated2015-12-12T09:03:59Z
local.identifier.scopusID2-s2.0-0012914125
CollectionsANU Research Publications

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