The White Dwarf Pareto: Tracing Mass Loss in Binary Systems
Sahar Shahaf

TL;DR
This paper introduces a new method using a Pareto distribution to analyze how binary interactions influence white dwarf masses, revealing significant mass loss and differences from isolated stars.
Contribution
It presents a novel application of a truncated Pareto profile to constrain white dwarf populations and their evolutionary history in binary systems.
Findings
White dwarfs in these binaries are ~20% less massive than isolated ones.
Progenitors lost 80-85% of their mass, with binary interactions increasing mass loss.
Typical white dwarf mass in the sample is ~0.55 Msun.
Abstract
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 interaction affects white dwarf masses. The binary mass ratio distribution is utilized for this purpose. Modeled as a truncated Pareto profile, this distribution provides insights into the populations' properties and evolutionary history. When applied to homogeneous samples of binaries with giant primaries of similar age, the distribution's shape constrains the fraction of white dwarf companions, the white dwarf mass distribution, and the properties of their progenitors. As a test case, this method is applied to a small spectroscopic sample of binaries in open clusters with red giant primaries and…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Scientific Research and Discoveries
