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The First Orbits of Six Wide Double Stars in the Solar Neighborhood Based on Gaia DR2 Observations
Authors:Kiyaeva  O. V.  Romanenko  L. G.
Affiliation:1.Pulkovo Astronomical Observatory, Russian Academy of Sciences, Pulkovskoe sh. 65, St. Petersburg, 196140, Russia
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Abstract:Astronomy Letters - The apparent motion parameter (AMP) method is designed to determine the orbits of wide pairs of double stars with orbital periods of hundreds and thousands of years. This is a...
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