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Asteroseismology and Stellar Pulsation feasibility at Dome C
Published online by Cambridge University Press: 05 January 2006
Abstract
Four site testing campaigns have already been conducted at Dome Cduring the local summers. A very reasonable extrapolation of theknowledge acquired on the atmospheric properties shows that broadband photometry could be exploited there for developingasteroseismology of many pulsating stars, including the solar-typeones, despite their very small oscillation amplitudes. This paperfocuses more specifically on the usual limiting factor inphotometry which is the scintillation.
- Type
- Research Article
- Information
- European Astronomical Society Publications Series , Volume 14: Dome C Astronomy and Astrophysics Meeting , 2005 , pp. 281 - 284
- Copyright
- © EAS, EDP Sciences, 2005