Poststarburst Quasars in the Sloan Digitial Sky Survey

Details Poststarburst Quasars in the Sloan Digitial Sky Survey Poststarburst Quasars in the Sloan Digitial Sky Survey

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.7817d&link_type=abstract

American Astronomical Society Meeting 203, #78.17; Bulletin of the American Astronomical Society, Vol. 35, p.1327

Astronomy and Astrophysics

Astronomy

Scientific paper

Poststarburst quasars are broad-lined AGN which also possess Balmer jumps and high-n Balmer absorption lines indicative of very luminous A-type stellar populations with ages on the order of 100 Myr. These "Q+A" objects may be an evolutionary stage in the transistion of ultraluminous infrared galaxies into normal quasars, or simply reveal a type of galaxy interaction that triggers both star formation and nuclear activity. I present initial results regarding the characterization of the Q+A population in Data Release One of the Sloan Digitial Sky Survey.
This work has been supported by NSF REU site grant AST 0097356.

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