activity
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

collaborators
Showing astro-ph.SRShow 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.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.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…

astro-ph.SR2024

Common envelopes at StanFest

Ilya Mandel, Ryosuke Hirai, Lewis Picker

We describe some of our group's recent work on common envelopes. Our goal is to understand the onset and outcomes of dynamically unstable mass transfer, including the properties of…

astro-ph.SR2024

Evolution of the Convective Core Mass during the Main Sequence

Minori Shikauchi, Ryosuke Hirai, Ilya Mandel

We construct a semi-analytical model that describes the convective core mass evolution of massive stars experiencing mass loss during the main-sequence stage. We first conduct a su…