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greywolf42 <[EMAIL PROTECTED]> wrote: : The angular velocity is calculated -- not observed. What's observed astrometrically is the projected angular velocity. That's adequate for the purpose of determining the 3-D orbit, except for a reflection ambiguity about the plane of the sky. Needless to say, that ambiguity is resolved if Doppler data are included. : One cannot determine inclination of a stellar orbit just from astrometry -- : even in the rare cases where you can watch and measure the describing of a : full ellipse by the orbiting body. The projection of an ellipse is still an : ellipse. You can get an upper bound to the central mass -- but not a : measurement of the central mass. You're confusing two very different problems: determining the mass of the system and determining the orbit. They are not the same. -- John F. Chandler [EMAIL PROTECTED]
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