Spectroscopic survey of Kepler stars: high-resolution observations of A- and F-type stars

Bibcode
2014IAUS..301..467N
DOI
10.1017/S1743921313015081
Niemczura, E.; Smalley, B.; Murphy, S.; Catanzaro, G.; Uytterhoeven, K.; Drobek, D.; Briquet, M.; De Cat, P.; Marcos-Arenal, P.; Pápics, P. I.; Gameiro, J. F. S.
Bibliographical reference

Precision Asteroseismology, Proceedings of the International Astronomical Union, IAU Symposium, Volume 301, pp. 467-468

Advertised on:
2
2014
Number of authors
11
IAC number of authors
1
Citations
2
Refereed citations
1
Description
Basic stellar parameters such as effective temperature, surface gravity, chemical composition, and projected rotational velocity, are important to classify stars and are crucial for successful asteroseismic modelling. However, the Kepler space data do not provide such information. Therefore, ground-based spectral and multi-colour observations of Kepler asteroseismic targets are necessary to complement the space data. For this purpose, in coordination with the KASC ground-based observational Working Groups, high-resolution spectroscopic data for more than 500 B, A, F and G-type stars were collected.
Type
Non-refereed

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