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
Since the pioneering works by Vandakurov (1967), Shibahashi (1979) and Tassoul (1980), asymptotic an...
CoRoT and Kepler observations of red giants reveal very rich spectra of non-radial solar- like oscil...
Context. Observations during the first long run (~150 days) in the exo-planet field of CoRoT increas...
The clear detection with CoRoT and Kepler of radial and non-radial solar-like oscillations in many r...
The non-radial oscillations discovered by CoRoT (see e.g. de Ridder et al. (2009)) and by Kepler(see...
Context. The advent of space-borne missions such as CoRoT or Kepler providing photometric data has b...
International audienceContext. The advent of space-borne missions such as CoRoT or Kepler providing ...
International audienceCoRoT and Kepler measurements reveal us that the amplitudes of solar-like osci...
CoRoT and Kepler observations of red giants reveal rich spectra of non-radial solar-like oscillation...
peer reviewedThe clear detection with CoRoT and KEPLER of radial and non-radial solar-like oscillati...
Context. Observations and analysis of solar-type oscillations in red-giant stars is an emerging aspe...
Today, asteroseismology is entering in its golden age thanks to the observations provided by the CoR...
International audienceContext. Convection in red giant stars excites resonant acoustic waves whose f...
Context. A growing number of solar-like oscillations has been detected in red giant stars thanks to ...
Corot and Kepler observations of red giants reveal rich spectra of non-radial solar-like oscillation...
Since the pioneering works by Vandakurov (1967), Shibahashi (1979) and Tassoul (1980), asymptotic an...
CoRoT and Kepler observations of red giants reveal very rich spectra of non-radial solar- like oscil...
Context. Observations during the first long run (~150 days) in the exo-planet field of CoRoT increas...
The clear detection with CoRoT and Kepler of radial and non-radial solar-like oscillations in many r...
The non-radial oscillations discovered by CoRoT (see e.g. de Ridder et al. (2009)) and by Kepler(see...
Context. The advent of space-borne missions such as CoRoT or Kepler providing photometric data has b...
International audienceContext. The advent of space-borne missions such as CoRoT or Kepler providing ...
International audienceCoRoT and Kepler measurements reveal us that the amplitudes of solar-like osci...
CoRoT and Kepler observations of red giants reveal rich spectra of non-radial solar-like oscillation...
peer reviewedThe clear detection with CoRoT and KEPLER of radial and non-radial solar-like oscillati...
Context. Observations and analysis of solar-type oscillations in red-giant stars is an emerging aspe...
Today, asteroseismology is entering in its golden age thanks to the observations provided by the CoR...
International audienceContext. Convection in red giant stars excites resonant acoustic waves whose f...
Context. A growing number of solar-like oscillations has been detected in red giant stars thanks to ...
Corot and Kepler observations of red giants reveal rich spectra of non-radial solar-like oscillation...
Since the pioneering works by Vandakurov (1967), Shibahashi (1979) and Tassoul (1980), asymptotic an...
CoRoT and Kepler observations of red giants reveal very rich spectra of non-radial solar- like oscil...
Context. Observations during the first long run (~150 days) in the exo-planet field of CoRoT increas...