activity
20242026
collaborators

6 papers

astro-ph.SR2026

Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements

Xiaozhen Yang, Xiaoting Fu, Mingjie Jian +10

Synthetic-template subtraction is widely used to measure chromospheric activity in large spectroscopic surveys. However, many solar-like FGK stars show systematically negative Ca I…

astro-ph.SR2026

Searching for Magnetic White Dwarfs in LAMOST DR10

Si-Cheng Yu, Juan-Juan Ren, Vitaly V. Neustroev +7

Magnetic white dwarfs (MWDs) are key to understanding the origin and evolution of magnetic fields in compact stars. While large spectroscopic surveys such as SDSS have greatly expa…

astro-ph.SR2025

The survey of DA double white dwarf candidates based on DESI EDR

Ziyue Jiang, Hailong Yuan, Zhongrui Bai +9

Mergers of double white dwarfs are considered significant potential progenitors of type Ia supernovae. Although there is no direct observational evidence to definitively determine…

astro-ph.SR2025

The Nature of Classical Be Star Outbursts: A Multi-Epoch Study of the Be system EPIC 202060631

Qing Gao, Hailong Yuan

Through cross-matching the ASASSN photometric light curves and LAMOST spectroscopic observations, we serendipitously captured a rare major outburst event from the Be star EPIC 2020…

astro-ph.SR2024

LAMOST J171013+532646: a detached short-period non-eclipsing hot subdwarf + white dwarf binary

Mingkuan Yang, Hailong Yuan, Zhongrui Bai +9

We present an analysis of LAMOST J171013.211+532646.04 (hereafter J1710), a binary system comprising a hot subdwarf B star (sdB) and a white dwarf (WD) companion. Multi-epoch spect…

astro-ph.SR2024

A potential mass-gap black hole in a wide binary with a circular orbit

Wang Song, Zhao Xinlin, Feng Fabo +28

Mass distribution of black holes identified through X-ray emission suggests a paucity of black holes in the mass range of 3 to 5 solar masses. Modified theories have been devised t…