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20232026
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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.SR2025

The Origins of Neutron-capture Elements In Globular Cluster M22

Muhammad Zeshan Ashraf, Wenyuan Cui, Hongjie Li

The chemical abundances of metal-poor stars in globular clusters provide important constraints on their evolutionary scenarios. Using both main r-process and weak r-process pattern…

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.SR2024

The Blue Horizontal-Branch Stars From the LAMOST Survey: Atmospheric Parameters

Jie Ju, Bo Zhang, Wenyuan Cui +4

Blue horizontal-branch (BHB) stars are crucial for studying the structure of the Galactic halo. Accurate atmospheric parameters of BHB stars are essential for investigating the for…

astro-ph.SR2024

The Value-added Catalog of OB Stars in LAMOST DR7

Zhicun Liu, Wenyuan Cui, Jiajia Gu +4

In this work, we update the catalog of OB stars based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) data release 7 and modified the OB stars selection c…

astro-ph.SR2024

Chemical abundances of 20 barium stars from the OHP spectra

Guochao Yang, Jingkun Zhao, Yanchun Liang +7

Based on the high resolution and high signal-to-noise spectra, we derived the chemical abundances of 20 elements for 20 barium (Ba-) stars. For the first time, the detailed abundan…

astro-ph.SR2024

Discovery of a new IW And-type dwarf nova with both tilted disk and tidal instability

Yongkang Sun, Xin Li, Qige Ao +6

IW And-type dwarf novae are anomalous Z Cam stars featured with outbursts happening during standstill states, which are not expected in the standard disk instability model. The phy…

astro-ph.SR2023

The measurement of masses of OB-type stars from LAMOST DR5

Zhenyan Huo, Zhicun Liu, Wenyuan Cui +5

The measurements of masses and luminosities of massive stars play an important role in understanding the formation and evolution of their host galaxies. In this work, we present th…