Atypical White Dwarfs in Open Clusters

arXiv:2610.10699 · astro-ph.SR, astro-ph.GA · Submitted 2026-10-07 · Read on arXiv

astro-ph.SR, astro-ph.GA

Submitted: 2026-10-07

Updated: 2026-10-07

Terminology

• Abundance — 3× in this paper · explained in 1 episode
• Consistency — 3× in this paper · explained in 3 episodes
• Core — 2× in this paper · explained in 2 episodes
• Metallicity — 2× in this paper · explained in 3 episodes
• Sloan Digital Sky Survey — 2× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Dark Energy Spectroscopic Instrument — 1× in this paper
• Degeneracy — 1× in this paper · explained in 3 episodes
• European Space Agency — 1× in this paper
• Mass Segregation — 1× in this paper · explained in 2 episodes
• Selection Bias — 1× in this paper · explained in 4 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• The Pan-STARRS1 Surveys
• The DESI Experiment Part I: Science,Targeting, and Survey Design
• A Framework for Linking Pre- and Post-Common Envelope Binary Properties with Star Clusters: The First Demonstration with a Massive White Dwarf+M Dwarf Binary in Alessi 12
• The white dwarf population of open clusters and their tidal tails. Tracers of contamination and stellar interactions
• The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper

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