collaborators

5 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.SR2025

The role of triple evolution in the formation of LISA double white dwarfs

Abinaya Swaruba Rajamuthukumar, Valeriya Korol, Jakob Stegmann +5

Galactic double white dwarfs will be prominent gravitational-wave sources for the Laser Interferometer Space Antenna (LISA). While previous studies have primarily focused on format…

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.SR2025

Carbon from massive binary-stripped stars over cosmic time: effect of metallicity

Jing-Ze Ma, Rob Farmer, Selma E. de Mink +1

The origin of carbon in the Universe remains uncertain. At solar metallicity, binary-stripped massive stars -- stars that lost their envelope through stable interaction with a comp…

astro-ph.IM2025

AREPO-IDORT: Implicit Discrete Ordinates Radiation Transport for Radiation Magnetohydrodynamics on an Unstructured Moving Mesh

Jing-Ze Ma, Rüdiger Pakmor, Stephen Justham +1

Radiation is crucial not only for observing astrophysical objects, but also for transporting energy and momentum. However, accurate on-the-fly radiation transport in astrophysical…