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Asteroseismology from Dome C

Published online by Cambridge University Press:  23 May 2007

N. Epchtein ,
M. Candidi  and
D.W. Kurtz
D.W. Kurtz*
Affiliation:
Centre for Astrophysics, University of Central Lancashire, Preston PR1 2HE, UK
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Abstract

This paper discusses the opportunities at Dome C for both photometric and spectroscopic asteroseismology. Dome C has two great advantages in this field: the first is the high percentage of superbly photometric skies; the second is the opportunity for long runs, a necessary requirement for asteroseismology. The potential of Dome C for asteroseismology is compared with existing ground-based networks and a potential spectroscopic networks, as well as with space missions.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 25: 1st ARENA Conference on "Large Astronomical Infrastructures at CONCORDIA, prospects and constraints for Antarctic Optical/IR Astronomy" , 2007 , pp. 95 - 101
Copyright
© EAS, EDP Sciences, 2007

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