Star Formation Analysis in Active Galactic Nuclei, Starburst, Ultraluminous Infrared, and Quasar Objects

Details Star Formation Analysis in Active Galactic Nuclei, Starburst, Ultraluminous Infrared, and Quasar Objects Star Formation Analysis in Active Galactic Nuclei, Starburst, Ultraluminous Infrared, and Quasar Objects

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..408...72h&link_type=abstract

The Starburst-AGN Connection. ASP Conference Series, Vol. 408, proceedings of the conference held 27-31 October 2008, at Shangha

Astronomy and Astrophysics

Astronomy

Scientific paper

The main goal of this work is to derive useful diagnostic tools that help to stablish a link between star formation phenomena and AGN activity. To this purpose, we use the log[L(12μm)/L(60μm)] ratio ≡ L(12,60), the luminosity and equivalent width of the 7.7μm PAH line, the star formation rate (SFR) and the size of the BRL. Our results show that these quantities, indeed, are intimately connected, supporting the current view of a link between AGN and starburst activity.

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