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Orbits of Galaxies in the LG and the LN

  In this section mainly two issues will be discussed, namely an extension of the evaluation of the optimizing methods from Section 5.3 to a considerably larger number of dimensions, and a brief physical interpretation of the solutions, including a slight alteration of the input data to get an improved fit between the observed and predicted radial velocities. But first, a presentation of the system of galaxies, the preferred cosmology, and some numerical parameters.

Trond Hjorteland
Mon Jul 5 02:59:28 MET DST 1999