Abstract

Recently the continuous energy distribution from the infrared to the radio region has been obtained for six Be stars, three of which are Be stars and three of which are shell stars. Analysis of these continuous energy distributions by Waters et al. in terms of a disk model has yielded the density distribution and the radial component of velocity in the circumstellar material. In this paper we determine the additional force, F x (r), exclusive of those arising from gravity, rotation, and the gas pressure gradient, which is required in this disk model to produce the radial component of velocity for each of the stars studied. We find that F x (r) for the three Be stars and the three shell stars has the same behavior

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