most citedDetection of Ubiquitous Circumbinary Matter in Hot Subdwarfs Formed from Common-Envelope Ejections

4 citations · 4 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025

First Time Observed M-Shaped Coronal Mass Ejection Associated with a Blowout Jet and an Extreme Ultraviolet Wave

Yu-Hu Miao, Lin-Hua Deng, Chao-Wei Jiang +8

The coronal blowout jet, extreme ultraviolet (EUV) wave and coronal mass ejection (CME) are common phenomena in the solar atmosphere. In this paper, we report the occurrence of an…

astro-ph.SR2025

A New Algol-type Binary with an Accretion disk

Tongyu He, Jiao Li, Xiaobin Zhang +10

We present a comprehensive photometric and spectroscopic analysis of the Algol-type binary \textit{Gaia} DR3 1892576067672499328. We identified the system as a spectroscopic binary…

astro-ph.SR2025

New symbiotic stars or candidates in LAMOST low resolution spectra

Yabing Zhao, Sufen Guo, Guoliang Lv +3

Symbiotic stars are among the most crucial binary systems for studying binary star interactions and Type Ia supernova progenitors. Based on the unique observational characteristics…

astro-ph.SR2025

Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-Resolution Survey

Sufen Guo, Mikhail Kovalev, Jiao Li +9

The period, mass ratio, eccentricity, and other orbital parameters are fundamental for investigating binary star evolution. However, the number of binaries with known orbital param…

astro-ph.SR2025

Surface brightness-color relations for red giant branch stars using asteroseismic radii and Gaia distances (the ARD method)

Jianping Xiong, Qiyuan Cheng, Xiaodian Chen +4

Aims. Asteroseismic radius and Gaia distance (ARD) method has been proposed to establish the SBCRs for late-type stars. Methods. We select Kepler RGB stars with high-precision aste…

astro-ph.SR20254 cited

Detection of Ubiquitous Circumbinary Matter in Hot Subdwarfs Formed from Common-Envelope Ejections

Jiangdan Li, Christian Wolf, Jiao Li +7

The formation of compact binary systems is largely driven by their evolution through a common envelope (CE) phase, crucial for understanding phenomena such as type Ia supernovae an…