The White Dwarf Pareto: Tracing Mass Loss in Binary Systems

The white dwarf mass distribution has been studied primarily at two extremes: objects that presumably evolved as single stars, and members of close binaries that likely underwent substantial interaction. This work considers the intermediate separation regime of  ∼1 au and demonstrates how binary int...

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Bibliographic Details
Published in:The Astrophysical Journal
Main Author: Sahar Shahaf
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adb156