Unravelling Active Galactic Nuclei

(2) MSSSO; (3) IPAC/Caltech; Australia; A.Y.K.N. Oshlack (1); F.J. Masci(3) ((1) University of Melbourne; M.J. Drinkwater (1); M.T. Whiting(1); P.J. Francis(2); R.L. Webster (1); USA)

arxiv: astro-ph/0005164 · v1 · submitted 2000-05-08 · 🌌 astro-ph

Unravelling Active Galactic Nuclei

A.Y.K.N. Oshlack (1) , R.L. Webster (1) , M.J. Drinkwater (1) , M.T. Whiting(1) , P.J. Francis(2) , F.J. Masci(3) ((1) University of Melbourne , Australia , (2) MSSSO

show 2 more authors

(3) IPAC/Caltech USA)

This is my paper

classification 🌌 astro-ph

keywords activeanalysisassociatedcolourscompletecontinuumdistanteither

0 comments

read the original abstract

A complete flat-spectrum radio-loud sample of AGN includes a significant fraction of Seyfert-like AGN including a NLS1. Analysis of their optical spectra suggests that the reddest continuum colours are either associated with AGN in nearby resolved galaxies, or distant quasars showing relatively narrow permitted emission lines.

This paper has not been read by Pith yet.

Unravelling Active Galactic Nuclei

discussion (0)