Observing solar-like oscillations
arXiv:0802.0531 · doi:10.1063/1.2818959
Abstract
The past few years have seen great progress in observing oscillations in solar-type stars, lying on or just above the main sequence. We review the most recent results, most of which were obtained using high-precision velocity measurements. We also briefly discuss observations of more evolved stars, namely G, K and M giants and supergiants.
Proc. of a conference on "Unsolved Problems in Stellar Physics", A Conference in Honour of Douglas Gough. AIP Conference Proceedings, Volume 948, pp. 117-124 (2007)
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