1996/08/16 by R. Cid Fernandes, Fernandes, R. Cid
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Solar and Space Plasma Dynamics #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9608110
6 pages, uses rmaaconf.sty. Also available at http://www.if.ufrgs.br/~cid To appear in "Starburst Activity in Galaxies", Rev. Mex. Astron. & Astroph. (1996)
arxiv created 1996/08/16 · openalex publication_date 1996/08/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
It is now eleven years since Terlevich & Melnick first proposed an `AGN without black-holes' model, an idea which since then evolved into what is now called the starburst model for AGN. This model has been the subject of much debate in the last decade, with observational evidence both for and against it further fuelling the controversy. Can we after all these years reach a veredictum on whether starbursts can power AGN? This contribution tries to answer this question reviewing the main achievements of the starburst model, its current status and future prospects.