Two contact binaries were identified in the tidal tails of young clusters, with one constrained to age less than 371 Myr and modeled as a deep low-mass-ratio system likely formed by rapid orbital hardening.
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W UMa-Type Contact Binaries in the Tidal Tails of Young Open Cluster COIN-Gaia 25 and Mamajek 4
Two contact binaries were identified in the tidal tails of young clusters, with one constrained to age less than 371 Myr and modeled as a deep low-mass-ratio system likely formed by rapid orbital hardening.