Probing the 2-D kinematic structure of early-type galaxies out to 3 effective radii

Details Probing the 2-D kinematic structure of early-type galaxies out to 3 effective radii Probing the 2-D kinematic structure of early-type galaxies out to 3 effective radii

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15...67p&link_type=abstract

Highlights of Astronomy, Volume 15, p. 67-67

Astronomy and Astrophysics

Astronomy

Scientific paper

We detail an innovative new technique for measuring the 2-D velocity
moments (rotation velocity, velocity dispersion and Gauss-Hermite
coefficients h3 and h4) using spectra from Keck
DEIMOS multi-object spectroscopic observations. The data are used to
reconstruct 2-D rotation velocity maps.

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