Coeval Bulge Growth in Powerful High Redshift Radio Galaxies

Details Coeval Bulge Growth in Powerful High Redshift Radio Galaxies Coeval Bulge Growth in Powerful High Redshift Radio Galaxies

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sacm.confe..28s&link_type=abstract

The Starburst-AGN Connection under the Multiwavelength Limelight, held 14-16 September 2011. Published online at http://www.scio

Computer Science

Scientific paper

High-redshift radio galaxies (HzRGs: L_3GHz>10^26 W/Hz and z>1) are unique markers of the most powerful galaxies in the early Universe, showing signatures of both powerful AGN activity and extreme star-formation. Our Spitzer project of a representative sample of 70 HzRGs demonstrated that these sources were hosted by massive galaxies, M>10^11 M_Sun, across 1

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