Magnetic activities and parameters of 43 flare stars in the GWAC archive
Guang-Wei Li, Chao Wu, Gui-Ping Zhou, Chen Yang, Hua-Li Li, Jie Chen,, Li-Ping Xin, Jing Wang, Hasitieer Haerken, Chao-Hong Ma, Hong-Bo Cai, Xu-Hui, Han, Lei Huang, Xiao-Meng Lu, Jian-Ying Bai, Xu-Kang Zhang, Xin-Li Hao,, Xiang-Yu Wang, Zi-Gao Dai, En-Wei Liang, Xiao-Feng Meng

TL;DR
This study analyzes 43 flare stars from the GWAC archive, identifying new active stars, characterizing flare activity, and assessing potential impacts on habitable planets through multi-instrument observations and light curve analysis.
Contribution
It provides the first comprehensive analysis of GWAC flare stars, combining optical, spectroscopic, and space-based data to characterize flare activity and stellar properties.
Findings
43 flare stars identified, including 19 new active stars.
Flares occur at a frequency of 0.5 to 9.5 per year.
Some flares may threaten habitable planets' ozone layers.
Abstract
In the archive of the Ground Wide Angle Camera (GWAC), we found 43 white light flares from 43 stars, among which, three are sympathetic or homologous flares, and one of them also has a quasi-periodic pulsation with a period of minutes. Among these 43 flare stars, there are 19 new active stars and 41 stars that have available TESS and/or K2 light curves, from which we found 931 stellar flares. We also obtained rotational or orbital periods of 34 GWAC flare stars, of which 33 are less than 5.4 days, and ephemerides of three eclipsing binaries from these light curves. Combining with low resolution spectra from LAMOST and the Xinglong 2.16m telescope, we found that are in the saturation region in the rotation-activity diagram. From the LAMOST medium-resolution spectrum, we found that Star \#3 (HAT 178-02667) has double H emissions which…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Solar and Space Plasma Dynamics · Astronomy and Astrophysical Research
