activity
20042026
most citedThe First Data Release (DR1) of the LAMOST general survey

862 citations · 1.1k across the 36 of their papers we have counts for

collaborators
Showing 2024Show all

12 papers · 1 filter

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.GA2024

When LAMOST meets Gaia DR3 Exploring the metallicity of open clusters

R. Zhang, Guo-Jian Wang, Yuxi +9

Context. Open clusters (OCs) are valuable probes of stellar population characteristics. Their age and metallicity provide insights into the chemical enrichment history of the Milky…

astro-ph.SR2024

TV Mon -- post mass transfer Algol type binary with Scuti pulsations in primary component

Mikhail Kovalev, Zhenwei Li, Jianping Xiong +4

We present a study of the detached eclipsing binary TV~Mon using spectra from the LAMOST medium-resolution survey and ASAS-SN, CoRoT photometry. We apply multiple-epochs spectral f…

astro-ph.SR2024

Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey

JiaRui Rao, HaiLiang Chen, JianPing Xiong +6

The measurement of atmospheric parameters is fundamental for scientific research using stellar spectra. The Chinese Space Station Telescope (CSST), scheduled to be launched in 2024…

astro-ph.CO2024★ 2 cited

Type Ia Supernovae from First-generation Stars

Zhenwei Li, Lifan Wang, Zhanwen Han +1

Type Ia Supernovae (SNe Ia) discovered at redshift are presumed to be produced from Population (Pop) I/II stars. {In this work, we investigate the production of SNe…

astro-ph.SR2024

Adiabatic Mass Loss In Binary Stars. IV. Low and Intermediate Mass Helium Binary Stars

Lifu Zhang, Hongwei Ge, Xuefei Chen +1

The unstable mass transfer situation in binary systems will asymptotically cause the adiabatic expansion of the donor star and finally lead to the common envelope phase. This proce…