Investigating the Physics of ISM in Type 2 QSOs

Details Investigating the Physics of ISM in Type 2 QSOs Investigating the Physics of ISM in Type 2 QSOs

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sptz.prop50309p&link_type=abstract

Spitzer Proposal ID #50309

Computer Science

Scientific paper

One of Spitzer's major contributions to the study of galaxy formation and evolution has been the detection of large numbers of obscured AGN. Spitzer found a large number of bigger and bolometrically brighter versions of Seyfert 2's, known as type 2 QSOs, whose existence had, until recently, only been theorized. Here, we propose to use IRS high resolution capabilities to perform a detailed analysis of the emission lines in a sample of six 0.3

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