Relations of rotation and chromospheric activity to stellar age for FGK dwarfs from Kepler and LAMOST
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2024
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| _version_ | 1866929226160013312 |
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| author | Ye, Lifei Bi, Shaolan Zhang, Jinghua Sun, Tiancheng Long, Liu Ge, Zhishuai Li, Tanda Zhang, Xianfei Chen, Xunzhou Li, Yaguang Zhou, Jianzhao Xiang, Maosheng |
| author_facet | Ye, Lifei Bi, Shaolan Zhang, Jinghua Sun, Tiancheng Long, Liu Ge, Zhishuai Li, Tanda Zhang, Xianfei Chen, Xunzhou Li, Yaguang Zhou, Jianzhao Xiang, Maosheng |
| contents | 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 the masses and ages of 52,321 FGK dwarfs, 47,489 chromospheric activity index $logR^{+}_{HK}$, 6,077 rotation period $P_{rot}$ and variability amplitude $S_{ph}$, based on data from LAMOST DR7, Kepler and Gaia DR3. We find a pronounced correlation among $P_{rot}$, age, and [Fe/H] throughout the main-sequence phase for F dwarfs. However, the decrease of $logR^{+}_{HK}$ over time is not significant except for those with [Fe/H] $<$ $-$0.1. For G dwarfs, both $P_{rot}$ and $logR^{+}_{HK}$ are reliable age probes in the ranges $\sim$ 2-11 Gyr and $\sim$ 2-13 Gyr, respectively. K dwarfs exhibit a prominent decrease in $logR^{+}_{HK}$ within the age range of $\sim$ 3-13 Gyr when the relation of $P_{rot}-τ$ is invalid. These relations are very important for promptly estimating the age of a vast number of stars, thus serving as a powerful tool in advancing the fields of exoplanet properties, stellar evolution, and Galactic-archaeology. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_15438 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Relations of rotation and chromospheric activity to stellar age for FGK dwarfs from Kepler and LAMOST Ye, Lifei Bi, Shaolan Zhang, Jinghua Sun, Tiancheng Long, Liu Ge, Zhishuai Li, Tanda Zhang, Xianfei Chen, Xunzhou Li, Yaguang Zhou, Jianzhao Xiang, Maosheng Solar and Stellar Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies 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 the masses and ages of 52,321 FGK dwarfs, 47,489 chromospheric activity index $logR^{+}_{HK}$, 6,077 rotation period $P_{rot}$ and variability amplitude $S_{ph}$, based on data from LAMOST DR7, Kepler and Gaia DR3. We find a pronounced correlation among $P_{rot}$, age, and [Fe/H] throughout the main-sequence phase for F dwarfs. However, the decrease of $logR^{+}_{HK}$ over time is not significant except for those with [Fe/H] $<$ $-$0.1. For G dwarfs, both $P_{rot}$ and $logR^{+}_{HK}$ are reliable age probes in the ranges $\sim$ 2-11 Gyr and $\sim$ 2-13 Gyr, respectively. K dwarfs exhibit a prominent decrease in $logR^{+}_{HK}$ within the age range of $\sim$ 3-13 Gyr when the relation of $P_{rot}-τ$ is invalid. These relations are very important for promptly estimating the age of a vast number of stars, thus serving as a powerful tool in advancing the fields of exoplanet properties, stellar evolution, and Galactic-archaeology. |
| title | Relations of rotation and chromospheric activity to stellar age for FGK dwarfs from Kepler and LAMOST |
| topic | Solar and Stellar Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2401.15438 |