Astrometric Measurements and Analysis of Double Star System BRT 376

Abstract

Using new telescope images and archival data, we investigated the positions and motions of the stars in double star system 06160-0745 BRT 376. We found that the two stars share nearly identical parallaxes and exhibit a low relative proper motion, suggesting they move together through space. Furthermore, their combined 3D velocity is less than the calculated escape velocity, indicating they are gravitationally bound rather than just physically near each other. These findings point to 06160-0745 BRT 376 being a true binary system. Future observations will help refine our understanding of its orbital path and further illuminate the nature of stars in close, interacting pairs.