collaborators

5 papers

astro-ph.SR2025

Starspots as the origin of ultrafast drifting radio bursts from an active M dwarf

Jiale Zhang, Hui Tian, Stefano Bellotti +16

Detecting coherent radio bursts from nearby M dwarfs provides opportunities for exploring their magnetic activity and interaction with orbiting exoplanets. However, it remains unce…

astro-ph.SR2025

Seismic test of the mass-radius relationship of hydrogen-atmospheric white dwarf stars

Tianqi Cang, Jiayi Zhang, Jian-Ning Fu +2

The pulsation of white dwarfs provides crucial information on stellar parameters for understanding the atmosphere and interior structure of these stars. In this study, we present a…

astro-ph.SR2025

Phase II of the LAMOST-Kepler/K2 Survey. II. Time Domain of Medium-resolution Spectroscopic Observations from 2018 to 2023

Mingfeng Qin, Jian-Ning Fu, Weikai Zong +11

The LAMOST-Kepler/K2 Medium-Resolution Spectroscopic Survey (LK-MRS) conducted time-domain medium-resolution spectroscopic observations of 20 LAMOST plates in the Kepler and K2 fie…

astro-ph.SR2025

Inactive longitude and superflare in the active single-lined pre-main sequence binary V2279 Cyg

Xueying Hu, Tianqi Cang, Jian-Ning Fu +7

Young, solar-like stars in the pre-main sequence (PMS) stage exhibit vigorous magnetic activity that significantly influences their circumstellar environments and the processes of…

astro-ph.SR2024

Magnetic field of the roAp star KIC~10685175: observations versus theory

Fangfei Shi, Huawei Zhang, Swetlana Hubrig +5

KIC 10685175 is a roAp star whose polar magnetic field is predicted to be 6 kG through a non-adiabatic axisymmetric pulsation theoretical model. In this work, we aim to measure the…