most citedA high fraction of close massive binary stars at low metallicity

22 citations · 39 across the 10 of their papers we have counts for

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astro-ph.SR2026

An upper limit on Galactic OB+black hole binaries from SDSS-V

J. Müller-Horn, H. -W. Rix, S. Shahaf +14

Binaries composed of a luminous OB star and a black hole (BH) are a key evolutionary link between massive stellar binaries and merging compact-object binaries, but only a handful a…

astro-ph.SR2026

Beyond what's observed: hierarchical inference of Gaia astrometric compact-object binaries

Natsuko Yamaguchi, Kareem El-Badry, Reed Essick +3

Astrometry from the Gaia mission has revealed a large and homogeneous population of binaries containing compact objects, including more than 3000 white dwarf--main sequence (WDMS)…

astro-ph.SR2026

Mass-dependent multiplicity fraction in low mass stars revealed by Gaia astrometry

Ben Pennell, Hans-Walter Rix, Kareem El-Badry +3

Stellar multiplicity at different orbital periods is probed by different techniques: radial velocities at the shortest periods, direct imaging at the longest, and astrometry in bet…

astro-ph.SR2026

Spectroscopic follow-up of compact object binary candidates from Gaia DR3: White dwarfs, neutron stars, black holes, and the parallax zeropoint

Kareem El-Badry, David W. Latham, Hans-Walter Rix +12

Astrometry and radial velocities (RVs) from Gaia DR3 yielded orbits for hundreds of thousands of binary systems, including several samples proposed to contain black holes (BHs), ne…

astro-ph.SR2026

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind

Johanna Müller-Horn, Kareem El-Badry, Andreas A. C. Sander +17

Binary interaction in massive stars is expected to produce a large population of intermediate-mass (- M) envelope-stripped stars, yet such objects have remained elusi…

astro-ph.SR2026★ 1 cited

IK Pegasi and the Double-merger Path to Type Ia Supernovae

Na'ama Hallakoun, Sahar Shahaf, Sagi Ben-Ami +3

Recent Gaia astrometry has revealed thousands of main-sequence + white-dwarf binaries (MS+WD) at separations of ~0.1-10 au, including a subset hosting unusually massive (>~0.8 Msun…

astro-ph.SR2026

Chemical Signatures of AGB Mass Transfer in Gaia White Dwarf Companions

Natsuko Yamaguchi, Kareem El-Badry, Henrique Reggiani +2

We present a homogeneous abundance analysis of 160 main-sequence stars in astrometric white-dwarf + main-sequence (WD+MS) binaries with orbits from Gaia DR3. These systems have AU-…

astro-ph.SR2025

The Silent Majority: The Interacting Post-Common-Envelope Binaries Underlying Cataclysmic Variables

Yarin Meir Shani, Na'ama Hallakoun, Sagi Ben-Ami +4

We analyze the orbital period distribution of post-common-envelope white-dwarf-main-sequence (WDMS) binaries by cross-matching the new spectroscopic Gaia DR3 WDMS catalog with TESS…

astro-ph.SR2025★ 22 cited

A high fraction of close massive binary stars at low metallicity

H. Sana, T. Shenar, J. Bodensteiner +74

At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, heavily impac…

astro-ph.SR2025★ 5 cited

Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts

Param Rekhi, Sahar Shahaf, Sagi Ben-Ami +4

The recently identified Gaia population of main-sequence--white dwarf (MS+WD) binaries at separations of , often with moderate eccentricities, is not readily re…

astro-ph.SR2025★ 11 cited

Population demographics of white dwarf binaries with intermediate separations: Gaia constraints on post-AGB mass transfer

Natsuko Yamaguchi, Kareem El-Badry, Sahar Shahaf

Astrometry from the Gaia mission has revealed a large population of white dwarf (WD) + main sequence (MS) binaries with periods of d. These systems have separations i…

astro-ph.SR2025

The initial-to-final mass relation of white dwarfs in intermediate-separation binaries

Oren Ironi, Sagi Ben-Ami, Na'ama Hallakoun +1

We examine the applicability of the initial-to-final mass relation (IFMR) for white dwarfs (WDs) in intermediate-separation binary systems (approximately 1 AU), using astrometric b…

astro-ph.SR2025

The White Dwarf Pareto: Tracing Mass Loss in Binary Systems

Sahar Shahaf

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 su…