activity
20132024
most citedMass and Age of Red Giant Branch Stars Observed with LAMOST and \emph{Kepler}

52 citations · 261 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR2024

Relations of rotation and chromospheric activity to stellar age for FGK dwarfs from Kepler and LAMOST

Lifei Ye, Shaolan Bi, Jinghua Zhang +9

The empirical relations between rotation period, chromospheric activity, and age can be used to estimate stellar age. To calibrate these relations, we present a catalog, including…

astro-ph.SR2023

Age of FGK Dwarfs Observed with LAMOST and GALAH: Considering the Oxygen Enhancement

Tiancheng Sun, Zhishuai Ge, Xunzhou Chen +11

Varying oxygen abundance could impact the modeling-inferred ages. This work aims to estimate the ages of dwarfs considering observed oxygen abundance. To characterize 67,503 LAMOST…

astro-ph.SR2022

Ages of Main-Sequence Turn-Off Stars from the GALAH Survey

Xunzhou Chen, Zhishuai Ge, Yuqin Chen +6

Main sequence turn-off (MSTO) stars are good tracers of Galactic populations since their ages can be reliably estimated from atmospheric parameters. Based on the GALAH survey, we u…

astro-ph.SR2020★ 49 cited

Magnetic Activity of F-, G-, and K-type Stars in the LAMOST-Kepler Field

Jinghua Zhang, Shaolan Bi, Yaguang Li +10

Monitoring chromospheric and photospheric indexes of magnetic activity can provide valuable information, especially the interaction between different parts of the atmosphere and th…

astro-ph.SR2017★ 52 cited

Mass and Age of Red Giant Branch Stars Observed with LAMOST and \emph{Kepler}

Yaqian Wu, Maosheng Xiang, Shaolan Bi +13

Obtaining accurate and precise masses and ages for large numbers of giant stars is of great importance for unraveling the assemblage history of the Galaxy. In this paper, we estima…

astro-ph.SR2016★ 13 cited

Ages of 70 dwarfs of three populations in the solar neighborhood: considering O and C abundances in stellar models

Z. S. Ge, S. L. Bi, Y. Q. Chen +5

Oxygen and carbon are important elements in stellar populations. Their behavior refers to the formation history of the stellar populations. C and O abundances would also obviously…

astro-ph.SR2016★ 15 cited

Asteroseismic analysis of two alpha-enhanced stars KIC 7976303 and KIC 8694723

Z. S. Ge, S. L. Bi, T. D. Li +5

We intent to use stellar models with and without alpha-enhancement, as well as asteroseismic analysis, to study two alpha-enhanced stars, KIC 7976303 and KIC 8694723. For the alpha…

astro-ph.SR2016★ 10 cited

Stellar Parameters of Main Sequence Turn-off Star Candidates Observed with the LAMOST and Kepler

Yaqian Wu, Maosheng Xiang, Xianfei Zhang +10

Main sequence turn-off (MSTO) stars have advantages as indicators of Galactic evolution since their ages could be robustly estimated from atmospheric parameters. Hundreds of thousa…

astro-ph.SR2015★ 12 cited

Asteroseismic analysis of Kepler target KIC 2837475

Wuming Yang, Zhijia Tian, Shaolan Bi +3

The ratios and of small to large separations of KIC 2837475 primarily exhibit an increase behavior in the observed frequency range. The calculations indicate that…

astro-ph.SR2014★ 3 cited

Precise determination of fundamental parameters of six exoplanet host stars and their planets

K. Liu, S. L. Bi, T. D. Li +3

The aim of this paper is to determinate the fundamental parameters of six exoplanet host (EH) stars and their planets. While techniques for detecting exoplanets yield properties of…

astro-ph.SR2014★ 1 cited

Exploring the sources of p-mode frequency shifts in the CoRoT target HD 49933

Zhie Liu, Shaolan Bi, Wuming Yang +5

The oscillations of the solar-like star HD 49933 have been observed thoroughly by CoRot. Two dozens of frequency shifts, which are closely related with the change in magnetic activ…

astro-ph.SR2013★ 16 cited

Asteroseismic analysis of the CoRoT target HD49933

Zhie Liu, Wuming Yang, Shaolan Bi +9

The frequency ratios and of HD 49933 exhibit an increase at high frequencies. This behavior also exists in the ratios of other stars, which is considered to result from the low sig…