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Chromospheric variabilities of M active stars based on Guoshoujing Telescope

Published online by Cambridge University Press:  06 January 2014

Q. F. Pi ,
L. Y. Zhang ,
J. R. Shi ,
H. Wu ,
Y. H. Zhao ,
A. L. Luo ,
J. K. Zhao ,
A. Y. Zhou ,
X. S. Fang  and
Lamost Collaboration
Q. F. Pi
Affiliation:
College of Science/Department of Physics, Guizhou University, Guiyang 550025, China email: [email protected]
L. Y. Zhang
Affiliation:
College of Science/Department of Physics, Guizhou University, Guiyang 550025, China email: [email protected]
J. R. Shi
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
H. Wu
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Y. H. Zhao
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
A. L. Luo
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
J. K. Zhao
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
A. Y. Zhou
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
X. S. Fang
Affiliation:
College of Science/Department of Physics, Guizhou University, Guiyang 550025, China email: [email protected]
Lamost Collaboration
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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Abstract

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For the M active catalogue of Guoshoujing Telescope (LAMOST), 933 sources are presented in at least two exposures. We found that many M active stars show chromospheric variability in the Ca II H, Hα, Hβ, and Hγ lines on short or long timescales.

Keywords

stars: Mstars: activitystars: chromospheresstars: spectra
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 433
Copyright
Copyright © International Astronomical Union 2014 

References

Cui, X. Q., Zhao, Y. H., Chu, Y. Q., et al., 2012, RAA, 12, 1197Google Scholar
Hilton, E. J., West, A. A., Hawley, S. L., et al., 2010, AJ, 140, 1402CrossRefGoogle Scholar
Hawley, S. L., Covey, K. R., Knapp, G. R., et al., 2002, AJ, 123, 3409CrossRefGoogle Scholar
Luo, A. L., Zhang, H. T., Zhao, Y. H., Zhao, G., et al., 2012, RAA, 12, 1243Google Scholar
Kruse, E. A., Berger, E., Knapp, G. R., et al., 2010, AJ, 722, 1352CrossRefGoogle Scholar
West, A. A., Morgan, D. P., Bochanski, J. J., et al., 2011, AJ, 141, 97Google Scholar
Zhang, L. Y., Shi, J. R., Zhao, J. K., Luo, A. L., et al., 2012, IAU294, 209CrossRefGoogle Scholar
Zhang, L. Y., Zhang, G. Y., Shi, J. R., Luo, A. L., et al., 2013, IAU298, in printGoogle Scholar
Zhao, G., Zhao, Y. H., Chu, Y. Q., et al., 2012, RAA, 12, 723Google Scholar