activity
20222026
most citedMass-Ratio Distribution of Binaries From the LAMOST-MRS Survey

12 citations · 23 across the 15 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution

Jiao Li, Changqing Luo, Hai-Liang Chen +16

Observationally, blue horizontal branch (BHB) stars are defined as hot stars occupying a characteristic region between the extreme blue horizontal branch and RR Lyrae variables in…

astro-ph.SR2026

First double red giant Algol system with active mass transfer

Mikhail Kovalev, Hailiang Chen, Sufen Guo +7

Double red giant stars are very important for studies of the stability of mass transfer, common-envelope evolution, and the formation of double white dwarfs with short orbital peri…

astro-ph.SR2026

Investigation of projected rotational velocities of Be-type stars in LAMOST DR7

Zhicun Liu, Jiao Li, Jiaming Liu +3

Stellar rotation plays a key role in the transfer of angular momentum, and a large sample of Be-type stars with reliable projected rotational velocities is crucial for understandin…

astro-ph.SR2026

Surface brightness-color relations for red giant branch stars: Observational constraints on metallicity effects using the ARD method

Jianping Xiong, Xiaodian Chen, Jiao Li +5

Aims: We aim to quantify the metallicity dependence of the SBCR for red giant branch (RGB) stars and to test the robustness of the relation using asteroseismic radii, Gaia distance…

astro-ph.SR2026

Empirical colour--effective temperature relations in the SDSS system from IRFM temperatures of GALAH and APOGEE stars

Zenghua Zhou, Luca Casagrande, Xiaobin Zhang +5

Reliable estimates of stellar effective temperature () are fundamental to stellar population studies and Galactic astrophysics. However, the majority of stars ob…

astro-ph.SR2026

Stellar Parameters and Orbital Period Estimates for Composite-Spectrum sdB+MS Binaries from LAMOST

Jiangdan Li, Jianping Xiong, Jiao Li +5

Hot subdwarf (sdB) stars in binary systems with main-sequence (MS) companions provide valuable insights into mass transfer and envelope ejection processes in binary evolution. Thei…

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★ 1 cited

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.SR2025★ 4 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…

astro-ph.SR2024★ 5 cited

The Red Supergiant Progenitor of the Type II Supernova 2024abfl

Jingxiao Luo, Lifu Zhang, Bing-Qiu Chen +9

Linkage between core-collapse supernovae (SNe) and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. $\mathrm{SN\…

astro-ph.SR2024

Discoveries and Properties of EL CVn-type Binaries in the TESS Survey

Jianping Xiong, Zhenwei Li, Jiao Li +5

EL CVn-type systems represent a rare evolutionary stage in binary star evolution, providing ideal laboratories for investigating stable mass transfer processes and the formation of…

astro-ph.SR2024

Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST

Tongyu He, Jiao Li, Jiangdan Li +8

Triple star systems are critical for understanding stellar dynamics and compact objects in astrophysics, yet confirmed hierarchical triples identified via spectroscopy remain limit…

astro-ph.SR2024★ 1 cited

A born ultramassive white dwarf-hot subdwarf super-Chandrasekhar candidate

Changqing Luo, Jiao Li, Chuanjie Zheng +16

Although supernovae is a well-known endpoint of an accreting white dwarf, alternative theoretical possibilities has been discussing broadly, such as the accretion-induced collapse…

astro-ph.SR2023

The Common Envelope Evolution Outcome. II. Short Orbital Period Hot Subdwarf B Binaries Reveal a Clear Picture

Hongwei Ge, Christopher A Tout, Ronald F Webbink +6

The common envelope evolution (CEE) is vital in forming short orbital period compact binaries. It covers many objects, such as double compact merging binaries, type Ia supernovae p…

astro-ph.SR2022★ 12 cited

Mass-Ratio Distribution of Binaries From the LAMOST-MRS Survey

Jiangdan Li, Jiao Li, Chao Liu +7

Binary evolution leads to the formation of important objects crucial to the development of astrophysics, but the statistical properties of binary populations are still poorly under…