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: http://www.eso.org/~chummel/oyster/manual/node82.html
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Fit all three masses, as well as the inclination of one of the pairs. That not any combination of orbital inclinations is allowed can be seen from the fact that the triple consists of two double-lined binaries and only one mass solution exists for a given inclination. Which inclination to vary depends on whether the adopted value of the other orbital inclination is larger or smaller than the true value.