High Z Galaxy Kinematics and Star Formation

Details High Z Galaxy Kinematics and Star Formation High Z Galaxy Kinematics and Star Formation

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21425703f&link_type=abstract

American Astronomical Society, AAS Meeting #214, #257.03; Bulletin of the American Astronomical Society, Vol. 41, p.758

Physics

Optics

Scientific paper

Studies of the spatially-resolved kinematics and star formation have just recently become feasible at high redshift, with near-IR integral field spectrometers at 10-m class telescopes. Together with adaptive optics (AO), we are now able to map those key properties on scales even as small as 1 kpc, providing new and unique constraints on the dynamical and physical processes driving the early evolution of massive galaxies. I will highlight results obtained with SINFONI+AO at the VLT and discuss implications on baryonic mass accretion and secular evolution at high redshift.

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