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20242026
most citedA high fraction of close massive binary stars at low metallicity

22 citations · 34 across the 10 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.SR2025

Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation

Adam Brček, Ryosuke Hirai, Ilya Mandel +1

Stars spend most of their lifetime on the main sequence (MS), where hydrogen burning establishes the internal chemical structure that governs the subsequent evolution. In massive s…

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.HE2025

What is the most massive gravitational-wave source?

Ilya Mandel

In the presence of significant measurement uncertainties, the events which appear to be the most extreme are very likely to be those exhibiting the greatest statistical fluctuation…

astro-ph.SR2025★ 1 cited

Rapid stellar and binary population synthesis with COMPAS: methods paper II

Ilya Mandel, Jeff Riley, Adam Boesky +13

The COMPAS public rapid binary population synthesis code has undergone a number of key improvements since the original COMPAS methods paper (Team COMPAS: Riley et al., 2022) was pu…

astro-ph.HE2025

Constraints on LIGO/Virgo Compact Object Mergers from Late-time Radio Observations

Ashna Gulati, Tara Murphy, Dougal Dobie +6

We present results from a search for radio afterglows of compact object mergers conducted with the Australian SKA Pathfinder. We used data from four epochs of the Rapid ASKAP Conti…

astro-ph.SR2025★ 11 cited

Common envelopes in massive stars III. The obstructive role of radiation transport in envelope ejection

Mike Y. M. Lau, Ryosuke Hirai, Daniel J. Price +2

We present 3D radiation hydrodynamics simulations of common-envelope (CE) evolution involving a 12 solar mass red supergiant donor and a 3 solar mass companion. Existing 3D simulat…