activity
20242026
collaborators

19 papers

astro-ph.GA2026

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae

M. Solar, M. J. Michałowski, J. Nadolny +11

Context. Study of cold molecular hydrogen gas (hereafter molecular gas) provides crucial insights into its interplay with star-forming regions. However, the connection between mole…

astro-ph.SR2026

A statistical study of the environmental age of core-collapse supernovae based on VLT/MUSE integral-field-unit spectroscopy

Qiang Xi, Ning-Chen Sun, Yihan Zhao +13

We aim to understand the progenitor channels of CCSNe via a statistical study of the ages of their environments. We compiled a large and minimally biased sample of 128 CCSNe discov…

astro-ph.SR2026

Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems

Abhishek Chattaraj, Jeff J. Andrews, Simone S. Bavera +14

With over two dozen detections in the Milky Way, double neutron stars (DNSs) provide a unique window into massive binary evolution. We use the POSYDON binary population synthesis c…

astro-ph.HE2026

Relative frequencies of core-collapse supernovae as a function of metallicity: observations vs theoretical predictions

Claudia P. Gutiérrez, Lluís Galbany, Joseph P. Anderson +4

Understanding supernova (SN) progenitors remains a major challenge in astrophysics, as it involves untangling the complex interplay between stellar physics (e.g., evolution, binari…

astro-ph.HE2026

Revealing the diversity of Type IIn supernova progenitors through their environments

Zexi Niu, Ning-Chen Sun, Emmanouil Zapartas +4

Type IIn supernovae (SNe IIn) are hydrogen-rich explosions embedded in dense circumstellar medium (CSM), which gives rise to their characteristic narrow hydrogen emission lines. Th…

astro-ph.SR2026

Disk-Regulated Mass Transfer Between Rotating Non-Degenerate Stars: Insights from Be and sdOB Binaries

Zepei Xing, Tassos Fragos, Vicky Kalogera +3

Mass transfer between non-degenerate stars is a fundamental but still poorly understood process in binary evolution. The commonly used rotationally limited accretion prescription i…