Shocks, plasma instabilities and undisturbed flows in parsec-scale jets

We discuss the relative contributions made by shocks, plasma instabilities and undisturbed flows to the emission and dynamics of compact, extragalactic jets. We summarize recent, in-depth studies of the jets in 3C 273 and 3C 345 and show that interpretation of these result calls for a new paradigm f...

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Main Authors: Lobanov, A, Roland, J
Format: Conference item
Published: 2002
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author Lobanov, A
Roland, J
author_facet Lobanov, A
Roland, J
author_sort Lobanov, A
collection OXFORD
description We discuss the relative contributions made by shocks, plasma instabilities and undisturbed flows to the emission and dynamics of compact, extragalactic jets. We summarize recent, in-depth studies of the jets in 3C 273 and 3C 345 and show that interpretation of these result calls for a new paradigm for the parsec-scale jets. Contrary to the commonly accepted views, the observed properties of the jets in these objects indicate that extragalactic jets remain relatively undisturbed on scales of similar to1-10 parsec. Farther on, on scales of similar to10-100 parsec, Kelvin-Helmholtz instabilities become the main contributor to the observed emission and kinematic changes. Relativistic shocks appear to be gaining prominence only on larger, sub-kiloparsec scales.
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spelling oxford-uuid:810bea49-e2c5-45da-a89b-9dd80604b2d02022-03-26T21:27:38ZShocks, plasma instabilities and undisturbed flows in parsec-scale jetsConference itemhttp://purl.org/coar/resource_type/c_5794uuid:810bea49-e2c5-45da-a89b-9dd80604b2d0Symplectic Elements at Oxford2002Lobanov, ARoland, JWe discuss the relative contributions made by shocks, plasma instabilities and undisturbed flows to the emission and dynamics of compact, extragalactic jets. We summarize recent, in-depth studies of the jets in 3C 273 and 3C 345 and show that interpretation of these result calls for a new paradigm for the parsec-scale jets. Contrary to the commonly accepted views, the observed properties of the jets in these objects indicate that extragalactic jets remain relatively undisturbed on scales of similar to1-10 parsec. Farther on, on scales of similar to10-100 parsec, Kelvin-Helmholtz instabilities become the main contributor to the observed emission and kinematic changes. Relativistic shocks appear to be gaining prominence only on larger, sub-kiloparsec scales.
spellingShingle Lobanov, A
Roland, J
Shocks, plasma instabilities and undisturbed flows in parsec-scale jets
title Shocks, plasma instabilities and undisturbed flows in parsec-scale jets
title_full Shocks, plasma instabilities and undisturbed flows in parsec-scale jets
title_fullStr Shocks, plasma instabilities and undisturbed flows in parsec-scale jets
title_full_unstemmed Shocks, plasma instabilities and undisturbed flows in parsec-scale jets
title_short Shocks, plasma instabilities and undisturbed flows in parsec-scale jets
title_sort shocks plasma instabilities and undisturbed flows in parsec scale jets
work_keys_str_mv AT lobanova shocksplasmainstabilitiesandundisturbedflowsinparsecscalejets
AT rolandj shocksplasmainstabilitiesandundisturbedflowsinparsecscalejets