Precision Asteroseismology Proceedings IAU Symposium No. 301, 2013

Abstract. 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 pote...

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Main Authors: J. A. Guzik, W. J. Chaplin, A. Pigulski, 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, D. Luong-van, Q. Liu, C. R. Pennypacker, Z. H. Shang, J. W. V. Storey, L. Z. Wang, L. F. Wang, H. G. Yang, X. Y. Yuan, D. G. York, X. Zhou, Z. H. Zhu
Other Authors: The Pennsylvania State University CiteSeerX Archives
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Language:English
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Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.637.4050
http://www.phys.unsw.edu.au/jacara/Papers/pdf/S1743921313014798a.pdf
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Summary:Abstract. 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. 1.