Outflows and shocks in compact radio sources

Details Outflows and shocks in compact radio sources Outflows and shocks in compact radio sources

2005-09-06

arxiv.org/abs/astro-ph/0509129v1

NewAstron.Rev.51:185-189,2007

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, to be published in Astronomische Nachrichten (proceedings of the Granada workshop on High Redshift Radio G

Scientific paper

10.1016/j.newar.2006.11.006

We report some key results from the optical emission line study of a complete sample of compact radio sources. We find strong evidence for jet-driven outflows in the circum-nuclear emission line gas namely: 1) highly broadened and blueshifted emission line components (up to 2000 km/s), 2) shock ionised gas (broader, shifted components), 3) consistency in the scales of the emission line gas and the radio source and 4) trends between the maximum outflow velocity and radio source size (and orientation). Full details can be found in Holt (2005).

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