THE MASSES OF SAN LUIS POTOSIHERICAL GALAXIES M32 A LIKELY APPLICATION
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UNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
Abstract
Our knowledge of the mass of early E galaxies is very limited. We propose that it is safer to estimate the mass of a spherical galaxy from the dispersion of its star velocities as determined by Minkowski for M32, and we analize the method with the help of