SUMMARY
Objects cataloged in dense fields are frequently composed of several blended sources. The authors show how the distribution of distances between the components of star pairs in a complete Gaia catalog population allows the authors to quantify the rate of widely separated double systems in the Galactic plane. The authors explain how the authors extrapolated the local binarity rate down to 50 au separations for stars closer than 500 pc to the Sun in Sect 6. Since the majority of the stars observed in the LMC correspond to the brightest stars in the Gaia data that the . . .
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