Are FeLoBAL quasars intrinsically young?

Details Are FeLoBAL quasars intrinsically young? Are FeLoBAL quasars intrinsically young?

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3276l&link_type=abstract

ATNF proposal C2365, Semester: April, 2010

Physics

Active Galactic Nuclei / Quasars, Atca

Scientific paper

The growth of bulges and central black holes in galaxies is one of the key questions of galaxy evolution. Why these co-evolve such that the tight black hole mass, bulge mass correlation is preserved with time is mostly untested though theoretical models suggest that feedback from a central quasar could achieve this by regulating the star formation process. The aim of these observations is to test whether the rare class of broad absorption line quasars called FeLoBALs is the best signpost for the start of this feedback phase. We wish to examine the molecular gas and dust continuum of a small sample of such sources to determine if their properties are akin to actively star forming ultraluminous infrared galaxies or whether they share similar infrared properties to "ordinary" high-z luminous quasars.

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