activity
20232026
most citedA high fraction of close massive binary stars at low metallicity

22 citations · 58 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

JWST observations of SN 2024abup: First Detection of CO in a broad-lined Type Ic Supernova and Constraints on r-process Nucleosynthesis

Manisha Shrestha, Lindsey A. Kwok, David J. Sand +42

SN 2024abup is a nearby broad-lined Type Ic supernova (SN Ic-bl) in NGC 0681 at a distance of 23.3 \pm 1.6 Mpc. As energetic explosions of massive stars, SNe Ic-bl are considered a…

astro-ph.HE2026

Jets from Scratch: Dynamo-Generated Poloidal Magnetic Fields in 3D Collapsar Simulations

Ho-Sang Chan, Ore Gottlieb, Jonatan Jacquemin-Ide +2

The origin of the large-scale poloidal magnetic field required to power relativistic jets in collapsars remains uncertain. While such a field may be inherited during PNS collapse,…

astro-ph.HE2025

Spinning into the Gap: Direct-Horizon Collapse as the Origin of GW231123 from End-to-End GRMHD Simulations

Ore Gottlieb, Brian D. Metzger, Danat Issa +3

GW231123, the most massive binary black hole (BH) merger observed to date, involves component BHs with masses inside the pair-instability mass gap and unusually high spins. This ch…

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

Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors

Aldana Grichener, Mathieu Renzo, Wolfgang E. Kerzendorf +7

One of the main challenges in modeling massive stars to the onset of core collapse is the computational bottleneck of nucleosynthesis during advanced burning stages. The number of…

astro-ph.HE2025★ 11 cited

r-Process Nucleosynthesis and Radioactively Powered Transients from Magnetar Giant Flares

Anirudh Patel, Brian D. Metzger, Jared A. Goldberg +3

We present nucleosynthesis and light-curve predictions for a new site of the rapid neutron capture process (-process) from magnetar giant flares (GFs). Motivated by observations…

astro-ph.HE2024

She's Got Her Mother's Hair: Unveiling the Origin of Black Hole Magnetic Fields through Stellar to Collapsar Simulations

Ore Gottlieb, Mathieu Renzo, Brian D. Metzger +2

Relativistic jets from a Kerr black hole (BH) following the core collapse of a massive star ("collapsar") is a leading model for gamma-ray bursts (GRBs). However, the two key ingre…

astro-ph.SR2024★ 1 cited

A Model for Eruptive Mass Loss in Massive Stars

Shelley J. Cheng, Jared A. Goldberg, Matteo Cantiello +3

Eruptive mass loss in massive stars is known to occur, but the mechanism(s) are not yet well-understood. One proposed physical explanation appeals to opacity-driven super-Eddington…

astro-ph.SR2024★ 22 cited

The Asteroseismic Imprints of Mass Transfer: A Case Study of a Binary Mass Gainer in the SPB Instability Strip

Tom Wagg, Cole Johnston, Earl P. Bellinger +3

We present new simulations investigating the impact of mass transfer on the asteroseismic signals of slowly pulsating B stars. We use MESA to simulate the evolution of a binary sta…

astro-ph.HE2024★ 2 cited

The Effects of -Process Enrichment in Hydrogen-Rich Supernovae

Anirudh Patel, Jared A. Goldberg, Mathieu Renzo +1

Core-collapse supernovae are candidate sites for the rapid neutron capture process (-process). We explore the effects of enrichment from -process nuclei on the light-curves o…

astro-ph.SR2023

Modelling time-dependent convective penetration in 1D stellar evolution

Cole Johnston, Mathias Michielsen, Evan H. Anders +7

1D stellar evolution calculations produce uncertain predictions for quantities like the age, core mass, core compactness, and nucleo-synthetic yields; a key source of uncertainty i…