Confirming the Tidal Tails of the Young Open Cluster Blanco 1 with TESS Rotation Periods

Blanco 1 is an ≈130 Myr open cluster located 240 pc from the Sun, below the Galactic plane. Recent studies have reported the existence of diffuse tidal tails extending 50–60 pc from the cluster center based on the positions and velocities measured by Gaia. To independently assess the reality and ext...

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Veröffentlicht in:	The Astrophysical journal 2024-12, Vol.977 (1), p.103
Hauptverfasser:	Sha, Lizhou, Vanderburg, Andrew M., Bouma, Luke G., Huang, Chelsea X.
Format:	Artikel
Sprache:	eng
Schlagworte:	Extrasolar planets Galactic clusters Kinematics Light curve Open clusters Open star clusters Rotation Stars Stellar ages Stellar photometry Stellar rotation Tidal tails
Online-Zugang:	Volltext
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