Outflows and shocks in compact radio sources

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

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006an....327..147h&link_type=abstract

Astronomische Nachrichten, Vol.327, Issue 2/3, p.147-150

Astronomy and Astrophysics

Astronomy

7

Galaxies: Active, Galaxies: Ism, Ism: Jets And Outflows, Ism: Kinematics And Dynamics.

Scientific paper

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 circumnuclear emission line gas namely: 1) highly broadened and blueshifted emission line components (up to 2000 km s-1), 2) shock ionized 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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