Image Details
Caption: Figure 2.
Candidate white dwarf escapees. Constant mass contours are shown from 0.2 to 1.3 M ⊙ (top right to bottom left), while age contours run horizontally for 50–800 Myr (top to bottom). Candidates selected for follow-up are labeled WD1–WD3 (green and blue). Orange points have total ages consistent with potential past cluster membership, but because their expected masses are below 1.0 M ⊙, they were not followed up. Black points are WDs that have kinematics consistent with having escaped the Hyades but appear to be too old for potential past cluster membership.
© 2023. The Author(s). Published by the American Astronomical Society.