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The thickness of H i in galactic discs under MOdified Newtonian Dynamics: theory and application to the Galaxy
Authors:F J Sánchez-Salcedo  K Saha  C A Narayan
Institution:Instituto de Astronomía, Universidad Nacional Autónoma de México, Apt. Postal 70 264, CP 04510, Mexico City, Mexico;Department of Physics, Indian Institute of Science, Bangalore 560012, India;Raman Research Institute, Bangalore 560080, India;Astronomisches Institut, Ruhr-Universitaet Bochum, Universitaetsstrasse 150, 44780 Bochum, Germany
Abstract:
Keywords:gravitation  Galaxy: disc  galaxies: haloes  galaxies: kinematics and dynamics  galaxies: structure
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