Project Details
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The Assembly of High Redshift Galaxies Probed by Imaging Spectroscopy

Subject Area Astrophysics and Astronomy
Term from 2005 to 2011
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 5448583
 
Final Report Year 2012

Final Report Abstract

Understanding how galaxies form and grow within the hierarchical framework of Cold Dark Matter remains a great challenge. Over the past six years, our ambitious program of near-infrared imaging spectroscopy with SINFONI at the ESO VLT and of millimeter interferometry at the IRAM Plateau de Bure of massive high-redshift star-forming galaxies has made substantial contributions, advancing our knowledge about the internal workings of galaxies in the early Universe. It has revealed the dynamics and properties of well over 100 distant galaxies in unprecendented detail, including the exciting discovery of a significant population of turbulent gas-rich disks at z∼2, whose evolution appears to be driven by efficient secular processes and whose star formation may be fueled by fairly smooth but rapid gas accretion via “cold flows.” The results are shedding new light on the origin of the massive spheroid and disk components of today’s galaxies, the connection between bulge and disk formation, and the physical processes driving mass accretion, star formation, chemical enrichment, and feedback from star formation and AGN activity at early cosmic times.

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