activity
20182026
most citedA potential mass-gap black hole in a wide binary with a circular orbit

33 citations · 137 across the 31 of their papers we have counts for

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24 papers · 1 filter

astro-ph.SR2026

Evolution of Stellar Activity and Habitable Zone (EATEN): III. X-ray Activity of Dwarfs in Open Clusters and Field Stars

Xue Li, Song Wang, Henggeng Han +3

Stellar X-ray emission serves as a direct diagnostic of coronal activity, which is fundamentally linked to coronal heating processes. It also strongly influences the atmospheres an…

astro-ph.SR2026

Flare waiting time as a novel proxy of stellar magnetic activity

Henggeng Han, Song Wang, Chuanjie Zheng +3

Stellar flares have long served as stellar magnetic activity tracers. The flare waiting time, defined as the interval between two consecutive flares, provides a valuable diagnostic…

astro-ph.SR2026

Unveiling the nature of G6096: a likely hierarchical triple system

Yinghao Xu, Xinlin Zhao, Song Wang +10

G6096 (Gaia DR3 609651611028044544) was recently reported as a wide ( days) and eccentric () binary possibly hosting a massive white dwarf or neutron star. In…

astro-ph.SR2026

Retarded Stellar Dynamo in Tidally Deformed M Dwarfs

Song Wang, Wenbo Li, Henggeng Han +3

Current studies of stellar dynamos primarily focus on spherical stars, leaving their behavior in distorted stars largely unexplored. We utilize stars of varying distortions to exam…

astro-ph.SR2026

Evolution of Stellar Activity and Habitable Zone II: Ca H&K Emissions of Late-type Dwarfs

Henggeng Han, Song Wang, Xue Li +3

Stellar chromospheric activity serves as a valuable proxy for estimating stellar ages, though its applicable range and accurate functional form are still debated. In this study, ut…

astro-ph.SR2025

Varying core-envelope coupling efficiency identified from stellar rotation--activity relation

Henggeng Han, Song Wang, Huiqin Yang +5

Core-envelope coupling provides a reasonable explanation of the spin-down stalling of stars in open clusters, which was not predicted by classical gyrochronology. However, it remai…

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.SR2025

Evolution of Stellar Activity and Habitable zone: I. Ultraviolet Emission of Dwarfs in Open Clusters and Field Stars

Xue Li, Song Wang, Jun Ma +3

Near-ultraviolet (NUV) radiation from dwarf stars plays a critical role in shaping the habitability of planetary systems, yet its long-term evolution across different spectral type…

astro-ph.SR2025

Revisiting the Li abundances of Stars with and without Detected Planets from the High Resolution Spectroscopy

Jinxiao Qin, Hong-Liang Yan, Wenyuan Cui +12

Whether the presence of planets affects the lithium (Li) abundance of their host stars is still an open question. To investigate the difference of the Li abundance between planet-h…

astro-ph.SR2025

Impact of Spectral Resolution on S-index and Its Application to Spectroscopic Surveys

Henggeng Han, Song Wang, Xue Li +2

Utilizing the PHOENIX synthetic spectra, we investigated the impact of spectral resolution on the calculation of -indices. We found that for spectra with a resolution lower than…

astro-ph.SR2025

"Frog-eyes" in Astronomy: Monitoring Binary Radial Velocity Variations Through A Pair of Narrow-Band Filters

Chuanjie Zheng, Yang Huang, Jifeng Liu +13

Spectroscopic observations are a crucial step in driving major discoveries in the era of time-domain surveys. However, the pace of current spectroscopic surveys is increasingly una…

astro-ph.SR2024

Photometric Stellar Parameters for 195,478 Kepler Input Catalog (KIC) Stars

Bowen Zhang, Yang Huang, Timothy C. Beers +9

The stellar atmospheric parameters and physical properties of stars in the Kepler Input Catalog (KIC) are of great significance for the study of exoplanets, stellar activity, and a…

astro-ph.SR2024

Revisiting the activity-rotation relation for evolved stars

Henggeng Han, Song Wang, Xue Li +2

The magnetic dynamo mechanism of giant stars remains an open question, which can be explored by investigating their activity-rotation relations with multiple proxies. By using the…

astro-ph.SR2024

Ultraviolet Photometry and Habitable Zones of Over 2700 Planet-Hosting Stars

Xue Li, Song Wang, Henggeng Han +1

The ongoing discovery of exoplanets has sparked significant interest in finding suitable worlds that could potentially support life. Stellar ultraviolet (UV; 100-3000 Å) radiation…

astro-ph.SR2024

Double-edged sword: the influence of tidal interaction on stellar activity in binaries

Yuedan Ding, Shidi Zhang, Henggeng Han +4

Using the LAMOST DR7 low-resolution spectra, we carried out a systematic study of stellar chromospheric activity in both single and binary stars. We constructed a binary sample and…

astro-ph.SR2024

Predicting photospheric UV emission from stellar evolutionary models

Song Wang, Xue Li, Henggeng Han +1

Stellar ultraviolet (UV) emission serves as a crucial indicator for estimating magnetic activity and evaluating the habitability of exoplanets orbiting stars. In this paper, we pre…

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…

astro-ph.SR2024★ 33 cited

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…

astro-ph.SR2024

Direct Method to Compute Doppler Beaming Factors in Binary Stars

Chuanjie Zheng, Yang Huang, Jifeng Liu +4

The Doppler beaming effect, induced by the reflex motion of stars, introduces flux modulations and serves as an efficient method to photometrically determine mass functions for a l…

astro-ph.SR2024★ 9 cited

Stellar X-ray activity and habitability revealed by ROSAT sky survey

Henggeng Han, Song Wang, Chuanjie Zheng +3

Using the homogeneous X-ray catalog from ROSAT observations, we conducted a comprehensive investigation into stellar X-ray activity-rotation relations for both single and binary st…

astro-ph.SR2024

Ultraviolet and Chromospheric activity and Habitability of M stars

Xue Li, Song Wang, Henggeng Han +4

M-type stars are crucial for stellar activity studies since they cover two types of magnetic dynamos and particularly intriguing for habitability studies due to their abundance and…

astro-ph.SR2022★ 14 cited

Stellar chromospheric activities revealed from the LAMOST-K2 time-domain survey

Henggeng Han, Song Wang, Yu Bai +3

By using the LAMOST time-domain survey data, we study stellar activities based on the lines for about 2000 stars in four 2 plates. Two indices, and…

astro-ph.SR2021★ 31 cited

LAMOST Time-Domain Survey: First Results of four 2 plates

Song Wang, Haotong Zhang, Zhongrui Bai +23

From Oct. 2019 to Apr. 2020, LAMOST performs a time-domain spectroscopic survey of four 2 plates with both low- and med-resolution observations. The low-resolution spectroscopic…

astro-ph.SR2018★ 32 cited

Do long-cadence data of {\it Kepler} satellite capture the basic properties of flares ?

Huiqin Yang, Jifeng Liu, Erlin Qiao +4

Flare research is becoming a burgeoning realm in the study of stellar activity due to the launch of {\it Kepler} in 2009. {\it Kepler} provides data with two time resolutions, i.e.…