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Asteroseismology from Dome A, Antarctica

Published online by Cambridge University Press:  18 February 2014

J. N. Fu ,
W. K. Zong ,
Y. Yang ,
A. Moore ,
M. C. B. Ashley ,
X. Q. Cui ,
L. L. Feng ,
X. F. Gong ,
J. S. Lawrence  and
D. Luong-Van
...Show all authors
J. N. Fu
Affiliation:
Department of Astronomy, Beijing Normal University, Beijing 100875, China
W. K. Zong
Affiliation:
Department of Astronomy, Beijing Normal University, Beijing 100875, China
Y. Yang
Affiliation:
Department of Astronomy, Beijing Normal University, Beijing 100875, China Department of Physics and Astronomy, Texas A&M University, College Station 77843, USA
A. Moore
Affiliation:
Caltech Optical Observatories, California Institute of Technology, Pasadena CA 91107, USA
M. C. B. Ashley
Affiliation:
School of Physics, University of New South Wales, NSW 2052, Australia
X. Q. Cui
Affiliation:
Nanjing Institute of Astronomical Optics and Technology, Nanjing 210042, China
L. L. Feng
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
X. F. Gong
Affiliation:
Nanjing Institute of Astronomical Optics and Technology, Nanjing 210042, China
J. S. Lawrence
Affiliation:
School of Physics, University of New South Wales, NSW 2052, Australia Australian Astronomical Observatory, NSW 1710, Australia
D. Luong-Van
Affiliation:
School of Physics, University of New South Wales, NSW 2052, Australia
Q. Liu
Affiliation:
National Astronomical Obs. of China, Chinese Academy of Sciences, Beijing 100012, China
C. R. Pennypacker
Affiliation:
Center for Astrophysics, Lawrence Berkeley National Laboratory, Berkeley, CA, USA
Z. H. Shang
Affiliation:
Tianjin Normal University, Tianjin 300074, China
J. W. V. Storey
Affiliation:
School of Physics, University of New South Wales, NSW 2052, Australia
L. Z. Wang
Affiliation:
National Astronomical Obs. of China, Chinese Academy of Sciences, Beijing 100012, China
L. F. Wang
Affiliation:
Department of Physics and Astronomy, Texas A&M University, College Station 77843, USA Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
H. G. Yang
Affiliation:
Polar Research Institute of China, Pudong, Shanghai 200136, China
X. Y. Yuan
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China Chinese Center for Antarctic Astronomy, Nanjing 210008, China
D. G. York
Affiliation:
Department of Astronomy and Astrophysics and Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA
X. Zhou
Affiliation:
National Astronomical Obs. of China, Chinese Academy of Sciences, Beijing 100012, China
Z. H. Zhu
Affiliation:
Department of Astronomy, Beijing Normal University, Beijing 100875, China
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Abstract

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Gattini and CSTAR have been installed at Dome A, Antarctica, which provide time-series photometric data for a large number of pulsating variable stars. We present the study for several variable stars with the data collected with the two facilities in 2009 to demonstrate the scientific potential of observations from Dome A for asteroseismology.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 409 - 410
Copyright
Copyright © International Astronomical Union 2014 

References

Liu, G. & Yuan, X. 2009, Acta Astron. Sinica, 50, 224Google Scholar
Moore, A., Yang, Y., Fu, J. N., et al. 2013, in: Burton, M. G., Cui, X., & Tothill, N. F. H. (eds.), Astrophysics from Antarctica, Proc. IAU Symposium No. 288 (Cambridge: Cambridge University Press), p. 34Google Scholar
Saunders, W., Lawrence, J. S., Storey, J. W. V., et al. 2009, PASP, 121, 976CrossRefGoogle Scholar
Zong, W. K., Fu, J. N., Niu, J. S., et al. 2013, AJ, submittedGoogle Scholar