Berkeley 86 and 87 lie at 1.7 kpc, are nearly coeval at 6 Myr with 3 Myr age spread, show patchy extinction, have extrapolated masses 519 and 1551 solar masses, and lack a common birthplace although Berkeley 87 likely formed with NGC 6913.
2002; Bressan et al
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Two young open clusters in Cygnus and their vicinity: combining multicolor photometry with Gaia DR3 astrometry
Berkeley 86 and 87 lie at 1.7 kpc, are nearly coeval at 6 Myr with 3 Myr age spread, show patchy extinction, have extrapolated masses 519 and 1551 solar masses, and lack a common birthplace although Berkeley 87 likely formed with NGC 6913.