activity
20052026
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 5.7k across the 75 of their papers we have counts for

collaborators

73 papers

astro-ph.SR2026

You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars

Thibault Lechien, Selma E. de Mink, Stephen Justham +3

The evolution of massive stars above 8 M depends critically on the amount of mixing above the convective core during the main sequence. However, current models typically ex…

astro-ph.SR2026★ 4 cited

Thermal-timescale accretion does not always yield critical rotation in mass gainers

Chen Wang, Mike Y. M. Lau, Xiang-Dong Li +7

Binary evolution plays a central role in producing rapidly rotating stars. Previous studies have shown that mass gainers in binaries can reach critical rotation after accreting onl…

astro-ph.IM2025

Dynamical binary interactions in the 2040s

Nadejda Blagorodnova, Ondřej Pejcha, Tomek Kamiński +15

Dynamical binary interactions such as common envelope (CE) evolution or stellar mergers are a critical phase in the formation of a wide variety of binary phenomena, ranging from bl…

astro-ph.SR2025

AREPO-RSG: Aspherical Circumstellar Material and Winds from Pulsating Dusty Red Supergiants in Global 3D Radiation Hydrodynamic Simulations

Jing-Ze Ma, Stephen Justham, Ruediger Pakmor +3

Recent observations have revealed a surprisingly large fraction of hydrogen-rich supernovae (SNe) interacting with dense confined circumstellar material (CSM), whose origin is heav…

astro-ph.HE2025★ 1 cited

Violent mergers revisited: The origin of the fastest stars in the Galaxy

Rüdiger Pakmor, Ken J. Shen, Aakash Bhat +12

Binary systems of two carbon-oxygen white dwarfs are one of the most promising candidates for the progenitor systems of Type Ia supernovae. Violent mergers, where the primary white…

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…