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New Ground-Based Observational Methods and Instrumentation for Asteroseismology

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Stellar Pulsations

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP,volume 31))

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Abstract

Space instrumentation like SOHO, MOST, CoRoT & Kepler has been and is being built to attain very high precision data to be used for asteroseismic analysis. Nonetheless, there is a very strong need for providing additional information, especially on mode identification. With this contribution I will review the efforts been put on new ground-based instrumentation and the methodology that can be used to achieve this aim.

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Notes

  1. 1.

    http://mwm.astro.puc.cl/mw/index.php/Main_Page

  2. 2.

    http://en.wikipedia.org/wiki/List_of_astronomical_interferometers_at_visible_and_infrared_wavelengths

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Acknowledgements

The author acknowledges financial support from projects AYA2009-08481-E and AYA2010-14840 from the Spanish Ministry of Science and Innovation.

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Correspondence to Pedro J. Amado .

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Amado, P.J. (2013). New Ground-Based Observational Methods and Instrumentation for Asteroseismology. In: Suárez, J., Garrido, R., Balona, L., Christensen-Dalsgaard, J. (eds) Stellar Pulsations. Astrophysics and Space Science Proceedings, vol 31. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-29630-7_27

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  • DOI: https://doi.org/10.1007/978-3-642-29630-7_27

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