activity
20242026
collaborators

5 papers

astro-ph.SR2026

The solar-like latitudinal distribution of flaring activities revealed by TESS, APOGEE and GALAH

Huiqin Yang, Shuai Liu, Yang Huang +2

Flare flux reflect contribution from active regions rather than the whole hemisphere of a star. Unlike the amplitude of light-curves caused by starspots, the flare detection is ind…

astro-ph.SR2025

Evaluating the chromospheric structure model of AD Leo using RH1.5D and magnetic field data

Shuai Liu, Jianrong Shi, Huigang Wei +4

Context. The interplay between surface magnetic topology and chromospheric heating in active M dwarfs remains poorly constrained, limiting our understanding of their magnetic cycle…

astro-ph.HE2025

LEIA discovery of the longest-lasting and most energetic stellar X-ray flare ever detected

Xuan Mao, He-Yang Liu, Song Wang +40

The Lobster Eye Imager for Astronomy (LEIA) detected a new X-ray transient on 2022 November 7, identified as a superflare event occurring on a nearby K-type giant star HD 251108. T…

astro-ph.SR2025

Flaring Activities of Fast Rotating Stars have Solar-like Latitudinal Distribution

Huiqin Yang, Xin Cheng, Jifeng Liu +6

The dynamo theory has always been one of the biggest mysteries in stellar physics. One key reason for its uncertainty is poor knowledge of the dynamo process on stars except the Su…

astro-ph.SR2024

Chromospheric modeling of the active M3V star G 80-21 with RH1.5D

Shuai Liu, Huigang Wei, Jianrong Shi +4

This study investigates the active regions of the M3.0V star G 80-21 using the observed data from the CARMENES project with synthetic spectra generated by the RH1.5D radiative tran…