Three contributions to Galaxy Dynamics: distant galaxy kinematics, mass, and M/L
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🌌 astro-ph
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bershadygalaxyandersengalaxieskinematicsmasscontributionscurves
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1) Rotation Curves and M/L Evolution for Galaxies to z=0.4, (Bershady, Haynes, Giovanelli, & Andersen) 2) Mass Estimates of Starbursting Galaxies: Line Widths versus Near-IR Luminosities (Jangren, Bershady, & Gronwall) 3) Galaxy Kinematics with Integral Field Spectroscopy (Andersen, Bershady)
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