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20162026
most citedCOSMIC Variance in Binary Population Synthesis

300 citations · 2.3k across the 64 of their papers we have counts for

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22 papers · 1 filter

astro-ph.SR2026

LISA's view of the Galactic Halo: forecasts for the Galactic double white dwarf population using Gaia data

Ann-Marsha Alexis, Katelyn Breivik

The population of close double white dwarfs (DWDs) in the Milky Way will make up the largest population of sources resolved by LISA, with a subset of the population having three-di…

astro-ph.SR2025

Gaia's promise to detect compact-object binaries: where we stand with the third data release

Chirag Chawla, Sourav Chatterjee, Katelyn Breivik

With its third data release (DR3), Gaia begins unveiling dormant candidate compact object (CO) binaries with luminous companions (LC) as predicted by several past theoretical studi…

astro-ph.SR2025★ 4 cited

Betelgeuse's Buddy: X-Ray Constraints on the Nature of Ori B

Anna J. G. O'Grady, Brendan O'Connor, Jared A. Goldberg +8

The d Long Secondary Period of Betelgeuse's optical lightcurve and radial velocity motivated the prediction of a low-mass stellar companion, expected to be at maximal a…

astro-ph.SR2025★ 1 cited

Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the dynamical companion to Orionis from HST

Jared A. Goldberg, Anna J. G. O'Grady, Meridith Joyce +10

Recently, two independent analyses have asserted that the cause of the Long Secondary Period (LSP) observed in the variability spectrum of our nearest red supergiant, Betelgeuse ($…

astro-ph.SR2025

Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback

Tom Wagg, Julianne J. Dalcanton, Mathieu Renzo +7

Core-collapse supernova feedback models in hydrodynamical simulations typically assume that all stars evolve as single stars. However, the majority of massive stars are formed in b…

astro-ph.SR2025★ 4 cited

Stellar ejection velocities from the binary supernova scenario: A comparison across population synthesis codes

Tom Wagg, David D. Hendriks, Mathieu Renzo +1

The vast majority of binary systems are disrupted at the moment of the first supernova, resulting in an unbound compact object and companion star. These ejected companion stars con…