LAMOST OBSERVATIONS OF FLARING M DWARFS IN THE KEPLER FIELD

被引:29
作者
Chang, H. -Y. [1 ]
Song, Y. -H. [2 ]
Luo, A. -L. [2 ]
Huang, L. -C. [1 ]
Ip, W. -H. [1 ,3 ]
Fu, J. -N. [4 ]
Zhang, Y. [5 ]
Hou, Y. -H. [5 ]
Cao, Z. -H. [2 ]
Wang, Y. -F. [5 ]
机构
[1] Natl Cent Univ, Inst Astron, 300 Jhongda Rd, Jhongli 32001, Taiwan
[2] Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China
[3] Macau Univ Sci & Technol, Space Sci Inst, Ave Wailong, Taipa, Macau, Peoples R China
[4] Beijing Normal Univ, Dept Astron, 19 Ave Xinjiekouwai, Beijing 100875, Peoples R China
[5] Chinese Acad Sci, Nanjing Inst Astron Opt & Technol, Natl Astron Observ, Nanjing 210042, Jiangsu, Peoples R China
基金
美国国家科学基金会;
关键词
stars: activity; stars: chromospheres; stars: flare; CHROMOSPHERIC ACTIVITY; STARS; FLARES; CATALOG;
D O I
10.3847/1538-4357/834/1/92
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A sample of the Large Sky Area Multi-Object Fibre Spectroscopic Telescope spectra of early-type M0-M3 dwarfs is compared with Kepler observations. It is found that M dwarfs with strong chromospheric emission in Ha have large flare activity in general. The rotational periods derived from the Kepler measurements have close correlations with the sizes of the flares, the power-law distribution index, and the equivalent widths of the H alpha emission. A clear trend exists for higher magnetic activities being detected in faster-rotating M dwarfs (rotation periods < 20 days).
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页数:7
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