activity
20132025
most citedNebular spectra of pair-instability supernovae

70 citations · 370 across the 12 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2025★ 24 cited

Explodability criteria for the neutrino-driven supernova mechanism

K. Maltsev, F. R. N. Schneider, I. Mandel +4

Massive stars undergoing iron core-collapse at the end of their evolution terminate their lives either in successful or failed supernovae (SNe). The physics of core-collapse supern…

astro-ph.HE2024★ 1 cited

Synthetic Light Curves and Spectra for the Photospheric Phase of a 3D Stripped-Envelope Supernova Explosion Model

Thomas Maunder, Fionntan P. Callan, Stuart A. Sim +2

We present synthetic light curves and spectra from three-dimensional (3D) Monte Carlo radiative transfer simulations based on a 3D core-collapse supernova explosion model of an ult…

astro-ph.HE2024★ 1 cited

The minimum neutron star mass in neutrino-driven supernova explosions

Bernhard Müller, Alexander Heger, Jade Powell

Supernova theory has struggled to explain the lightest known neutron star candidate with an accurate mass determination, the companion in the eccentric comp…

astro-ph.SR2023★ 1 cited

On the Core-Collapse Supernova Explanation for LAMOST J1010+2358

S K Jeena, Projjwal Banerjee, Alexander Heger

Low-metallicity very massive stars with an initial mass of -- are expected to end their lives as pair-instability supernovae (PISNe). The abundance p…

astro-ph.HE2020★ 30 cited

Properties of gamma-ray decay lines in 3D core-collapse supernova models, with application to SN 1987A and Cas A

A. Jerkstrand, A. Wongwathanarat, H. -T. Janka +8

Comparison of theoretical line profiles to observations provides important tests for supernova explosion models. We study the shapes of radioactive decay lines predicted by current…

astro-ph.SR2017★ 1 cited

Simulations of Electron Capture and Low-Mass Iron Core Supernovae

B. Müller, S. Wanajo, H. -Th. Janka +3

The evolutionary pathways of core-collapse supernova progenitors at the low-mass end of the spectrum are beset with major uncertainties. In recent years, a variety of evolutionary…