{ "id": "2401.15438", "version": "v1", "published": "2024-01-27T15:12:50.000Z", "updated": "2024-01-27T15:12:50.000Z", "title": "Relations of rotation and chromospheric activity to stellar age for FGK dwarfs from Kepler and LAMOST", "authors": [ "Lifei Ye", "Shaolan Bi", "Jinghua Zhang", "Tiancheng Sun", "Liu Long", "Zhishuai Ge", "Tanda Li", "Xianfei Zhang", "Xunzhou Chen", "Yaguang Li", "Jianzhao Zhou", "Maosheng Xiang" ], "categories": [ "astro-ph.SR", "astro-ph.EP", "astro-ph.GA" ], "abstract": "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 $P_{rot}-\\tau$ 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.", "revisions": [ { "version": "v1", "updated": "2024-01-27T15:12:50.000Z" } ], "analyses": { "keywords": [ "fgk dwarfs", "rotation period", "estimate stellar age", "chromospheric activity index", "lamost dr7" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }