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20032026
most citedThe massive binary companion star to the progenitor of supernova 1993J

329 citations · 7.7k across the 152 of their papers we have counts for

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astro-ph.SR2026

SN 2023fyq: direct detection of a Type Ibn supernova progenitor and its multi-wavelength environmental constraints

Xinyi Hong, Ning-Chen Sun, Yali Shao +9

Context. Type Ibn supernovae (SNe) are characterized by narrow helium emission lines arising from ejecta-circumstellar medium interaction, yet their progenitors remain debated, wit…

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

Direct Detection of Type II-P Supernova Progenitors with the and CSST Surveys

Junjie Wu, Ning-Chen Sun, Zexi Niu +14

Identifying and characterizing supernova (SN) progenitor stars remains a central yet difficult goal in SN research, limited by archival images lacking sufficient depth or spatial r…

astro-ph.SR2025★ 4 cited

An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi

Yi Yang, Xudong Wen, Lifan Wang +18

The death of massive stars is triggered by an infall-induced bounce shock that disrupts the star. How such a shock is launched and propagates through the star is a decade-long puzz…

astro-ph.SR2025

SN 2024aecx: a fast-evolving Type IIb supernova with a prominent shock-cooling peak

Qiang Xi, Ning-Chen Sun, David Aguado +36

SN 2024aecx is a nearby (11 Mpc) Type IIb SN discovered within 1 d after explosion. In this paper we report high-cadence photometric (typically 0.51 day) and spec…

astro-ph.SR2025

A late-time view of the progenitor candidates of the Type II-P SN 2009ib and SN 2012ec

Yi-Han Zhao, Xinyi Hong, Ning-Chen Sun +3

The progenitors of Type II-P supernovae (SNe) are generally considered to be red supergiants; however, the so-called "red supergiant problem" indicates that a deeper investigation…