Abstract
CoRoT photometric measurements of asteroseismic targets need complementary ground-based spectroscopic observations. We are using the planet-hunter HARPS spectrograph attached to the 3.6m-ESO telescope in the framework of two consecutive Large Programmes. We discuss its use to study line-profile variations and we report on a specific result obtained for the ı Sct star HD 170699.
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CITATION STYLE
Poretti, E., Rainer, M., Mantegazza, L., Floquet, M., Mathias, P., Amado, P., & Aerts, C. (2013). The spectroscopic observations of corot asteroseismic targets with harps. In Astrophysics and Space Science Proceedings (Vol. 31, pp. 39–42). Springer Netherlands. https://doi.org/10.1007/978-3-642-29630-7_7
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