Adiabatic solar-like oscillations in red giant stars
arXiv:1108.4777 · doi:10.1007/978-3-642-18418-5_3
Abstract
Since the detection of non-radial solar-like oscillation modes in red giants with the CoRoT satellite, the interest in the asteroseismic properties of red giants and the link with their global properties and internal structure is substantially increasing. Moreover, more and more precise data are being collected with the space-based telescopes CoRoT and Kepler. In this paper we present a survey of the most relevant theoretical and observational results obtained up to now concerning the potential of solar-like oscillations in red giants.
Proc. of the workshop "Red Giants as Probes of the Structure and Evolution of the Milky Way" (Roma, 15-17 Nov 2010), Astrophysics and Space Science Proceedings, ISBN 978-3-642-18417-8 (eds. A. Miglio, J. Montalban, A. Noels). Part of RedGiantsMilkyWay/2011/ proceedings available at http://arxiv.org/html/1108.4406v1
References in corpus (3)
Cited by in corpus (10)
- Age dissection of the Milky Way discs: red giants in the Kepler field
- Chronologically dating the early assembly of the Milky Way
- Period spacings in red giants; III. Coupling factors of mixed modes
- Asteroseismology of red giants: from analysing light curves to estimating ages
- Models of red giants in the CoRoT asteroseismology fields combining asteroseismic and spectroscopic constraints
- Asteroseismology of overmassive, undermassive, and potential past members of the open cluster NGC6791
- Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars
- Solar-like oscillating stars as standard clocks and rulers for Galactic studies
- Coralie radial velocity search for companions around evolved stars (CASCADES) II. Seismic masses for three red giants orbited by long-period massive planets
- Physical interpretation of the oscillation spectrum on the RGB and AGB