Star-Forming AGN Host Galaxies

Abstract

The symbiosis of nuclear activity and star-formation in galaxies, as manifested in their spectral energy distributions (SEDs) is reviewed. Attention is drawn to an Hertzsprung-Russell diagram-equivalent for such objects, as well as to the importance of the SEDs in cosmological context.

Invited review for FIRSED2000 Workshop (Groningen, April 2000)

References in corpus (1)

• The obscured mid-infrared continuum of NGC 4418: a dust- and ice-enshrouded AGN

Cited by in corpus (5)

• The Physical Connections Among IR QSOs, PG QSOs and Narrow-Line Seyfert 1 Galaxies
• Associated absorption in radio quasars. I. C IV absorption and the growth of radio sources
• High-excitation molecular gas in local luminous AGN hosts
• A Sample of IRAS Infrared-Selected Seyfert 1.5 Galaxies: Infrared-Color $\alpha (60,25)$ Dominated Eigenvector 1
• Host Galaxy Evolution in Radio-Loud AGN