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most citedBinary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729

2 citations · 2 across the 12 of their papers we have counts for

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astro-ph.SR2026

A prolonged plateau-to-tail transition in the Type II supernova SN2025abyc

Luhan Li, Bo Wang, Jujia Zhang +6

We present optical photometric and spectroscopic observations of the Type II supernova SN2025abyc. During the optically thick phase between approximately 10 and 70 d after explosio…

astro-ph.SR2026

The double white dwarf merger model for the progenitors of SN 2021yfj-like events

Dongdong Liu, Chengyuan Wu, Takashi J. Moriya +4

Context. Recently, a new class of supernovae with prominent narrow emission features of Si, S and Ar has been reported, i.e. SN 2021yfj-like events (SNe Ien). Their progenitor orig…

astro-ph.SR2026

Surrogate models for type II supernovae: Probing low-energy explosions and interaction-free regimes

Zhengyang Zhang, Shuai Zha, Nikhil Sarin +3

To address the computational bottleneck of analyzing type II supernova samples from surveys such as the Legacy Survey of Space and Time, we present two STELLA-based neural-network…

astro-ph.SR2026

Elemental Abundances from Off-center Carbon Burning in Accreting CO White Dwarfs: Implications for SN 2021yfj-like events

Chengyuan Wu, Dongdong Liu, Takashi J. Moriya +3

SN 2021yfj is a recently discovered interacting supernova that exhibits narrow emission lines of Si, S, and Ar, indicating the presence of circumstellar material (CSM) enriched wit…

astro-ph.SR2025

Evolution Models of CO WD -- AGB Star Merger Remnants

Chengyuan Wu, Heran Xiong, Shi Jia +2

Common envelope evolution is a critical but still poorly understood phase in binary evolution. It plays a key role in forming close binaries such as hot subdwarfs, double white dwa…

astro-ph.SR2025

Helium-burning blue large-amplitude pulsators: A Population Study with BPASS

Zhengyang Zhang, Conor M. Byrne, Chengyuan Wu +1

Blue Large-Amplitude Pulsators (BLAPs) are a class of radially pulsating stars with effective temperatures ranging from 20,000 to 35,000 K and pulsation periods between 7 and 75 mi…

astro-ph.SR2025★ 2 cited

Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729

Zhengyang Zhang, Chengyuan Wu, Xianfei Zhang +2

Blue Large-Amplitude Pulsators (BLAPs) represent a recently identified class of pulsating stars distinguished by their short pulsation periods ( minutes) and asymmetric lig…

astro-ph.SR2024

He-accreting oxygen-neon white dwarfs and accretion-induced collapse events

Zhengyang Zhang, Chengyuan Wu, Amar Aryan +3

It has been widely accepted that mass-accreting white dwarfs (WDs) are the progenitors of Type Ia supernovae or electron-capture supernovae. Previous work has shown that the accret…