The NASA K2 mission that succeeded the nominal Kepler mission observed several hundred thousand stars during its operations. While most of the stars were...
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PublicaciónMulti-campaign asteroseismic analysis of eight solar-like pulsating stars observed by the K2 mission
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PublicaciónOn the Characterization of GJ 504: A Magnetically Active Planet-host Star Observed by the Transiting Exoplanet Survey Satellite (TESS)
We present the results of the analysis of the photometric data collected in long- and short-cadence mode by the Transiting Exoplanet Survey Satellite for GJ 504...
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PublicaciónOscillating red giants in eclipsing binary systems: empirical reference value for asteroseismic scaling relation
The internal structures and properties of oscillating red-giant stars can be accurately inferred through their global oscillation modes (asteroseismology)...
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PublicaciónOscillation mode frequencies of 61 main-sequence and subgiant stars observed by Kepler
Context. Solar-like oscillations have been observed by Kepler and CoRoT in several solar-type stars, thereby providing a way to probe the stars using...
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PublicaciónOscillation mode linewidths and heights of 23 main-sequence stars observed by Kepler
Context. Solar-like oscillations have been observed by Kepler and CoRoT in many solar-type stars, thereby providing a way to probe the stars using...
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PublicaciónOscillation mode linewidths and heights of 23 main-sequence stars observed by Kepler (Corrigendum)
Not Available
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PublicaciónOscillations in the Sun with SONG: Setting the scale for asteroseismic investigations
Context. We present the first high-cadence multiwavelength radial-velocity observations of the Sun-as-a-star, carried out during 57 consecutive days using the...
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PublicaciónOvershooting and semiconvection: structural changes and asteroseismic signatures
Overshooting and semiconvection are two poorly known mechanisms which affect the extent and the efficiency of chemical mixing outside classical convection zones...
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PublicaciónPeriodic mass-loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD 50064
Aims: We aim to interpret the photometric and spectroscopic variability of the luminous blue variable supergiant HD 50064 (V = 8.21). Methods: CoRoT space...