Abstract
Photometric and kinematic observations of elliptical galaxies are not sufficient to determine the complete phase-space distribution function of the Galaxy. In general, many possible distribution functions are consistent with the available observations; statistical mechanics and information theory suggest that the most natural of these are the ones with the largest entropy. It is shown how to construct the maximum-entropy distribution function consistent with given emissivity and potential distributions and a given set of kinematic observations. As examples, the maximum-entropy models consistent with two common spherical luminosity distributions, the Plummer model and the de Vaucouleurs R exp 1/4 model, are constructed. Maximum-entropy models offer a flexible and straightforward approach to modeling galaxies from limited observational data. 13 references.
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