Observations of solar-like oscillations
arXiv:0705.1376 · doi:10.1553/cia150s106
Abstract
There has been tremendous progress in observing oscillations in solar-type stars. In a few short years we have moved from ambiguous detections to firm measurements. We briefly review the recent results, most of which have come from high-precision Doppler measurements. We also review briefly the results on giant and supergiant stars and the prospects for the future.
Invited review talk at the "Vienna Workshop on the Future of Asteroseismology", 20-22 September 2006, to appear in Communications in Asteroseismology
Cited by in corpus (8)
- Asteroseismology and Interferometry
- The amplitude of solar oscillations using stellar techniques
- Gaussian Process Modelling of Asteroseismic Data
- Photometric Oscillations of Low Luminosity Red Giant Stars
- The Current Status of Asteroseismology
- Solar-like oscillations in a metal-poor globular cluster with the HST
- Fourier Analysis of Gapped Time Series: Improved Estimates of Solar and Stellar Oscillation Parameters
- A search for solar-like oscillations in K giants in the globular cluster M4