most citedA seven-Earth-radius helium-burning star inside a 20.5-min detached binary

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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

Stellar Parameters and Orbital Period Estimates for Composite-Spectrum sdB+MS Binaries from LAMOST

Jiangdan Li, Jianping Xiong, Jiao Li +5

Hot subdwarf (sdB) stars in binary systems with main-sequence (MS) companions provide valuable insights into mass transfer and envelope ejection processes in binary evolution. Thei…

astro-ph.SR2026

SN2024abfl: A Low-Luminosity Type IIP Supernova at the Low-Mass End of Core Collapse

Luhan Li, Jujia Zhang, Zeyi Zhao +8

We present optical photometric and spectroscopic observations of the low-luminosity (LL) Type IIP supernova SN\,2024abfl. The distance to its host galaxy is highly uncertain, with…

astro-ph.SR2023★ 16 cited

A seven-Earth-radius helium-burning star inside a 20.5-min detached binary

Jie Lin, Chengyuan Wu, Heran Xiong +28

Binary evolution theory predicts that the second common envelope (CE) ejection can produce low-mass (0.32-0.36 Msun) subdwarf B (sdB) stars inside ultrashort-orbital-period binary…