Over the past decade, space-based asteroseismology has played an important role in the characterization of host stars and their planetary systems. The future looks even brighter, with space missions such as TESS and PLATO ready to take on this legacy. In this talk, I start by introducing the main observational features of convection-driven, or solar-like, oscillations. I then review current key synergies between asteroseismology and exoplanetary science, after which I present an outlook on potential future synergies. And now that TESS science data have been available for a few years, I find it relevant to talk about the prospects of conducting asteroseismology of exoplanet-host stars with TESS and also to look at some of the mission's early...
The Transiting Exoplanet Survey Satellite (TESS) is a NASA Astrophysics Explorer mission. Following ...
It is well known that asteroseismology is the unique technique permitting the study of the internal ...
Studying the internal structure of exoplanet-host stars compared to that of similar stars without de...
Space-based asteroseismology has been playing an important role in the characterization of exoplanet...
The detection of solar-like oscillations in thousands of cool stars enabled by the ultra-precise pho...
We propose a new synergic strategy that merges the potential of asteroseismology with solar space cl...
Abstract. The measurement of oscillations excited by surface convection is a powerful method to stud...
Today, asteroseismology is entering in its golden age thanks to the observations provided by the CoR...
Asteroseismology, the study of intrinsic oscillations in stars, can reveal fundamental properties of...
© 2022. The Author(s). Published by the American Astronomical Society..We present an analysis of the...
New observations of stellar pulsations, particularly from the CoRoT and Kepler space missions, have ...
A new generation of space-based observations has revolutionised the field of asteroseismology. In th...
© The Authors 2023.Context. The Transiting Exoplanet Survey Satellite (TESS) mission has provided ph...
The characterization of exoplanets conditions cannot be based solely on the knowlegde of the planeta...
The study of stellar oscillations - asteroseismology - has revolutionized our understanding of the p...
The Transiting Exoplanet Survey Satellite (TESS) is a NASA Astrophysics Explorer mission. Following ...
It is well known that asteroseismology is the unique technique permitting the study of the internal ...
Studying the internal structure of exoplanet-host stars compared to that of similar stars without de...
Space-based asteroseismology has been playing an important role in the characterization of exoplanet...
The detection of solar-like oscillations in thousands of cool stars enabled by the ultra-precise pho...
We propose a new synergic strategy that merges the potential of asteroseismology with solar space cl...
Abstract. The measurement of oscillations excited by surface convection is a powerful method to stud...
Today, asteroseismology is entering in its golden age thanks to the observations provided by the CoR...
Asteroseismology, the study of intrinsic oscillations in stars, can reveal fundamental properties of...
© 2022. The Author(s). Published by the American Astronomical Society..We present an analysis of the...
New observations of stellar pulsations, particularly from the CoRoT and Kepler space missions, have ...
A new generation of space-based observations has revolutionised the field of asteroseismology. In th...
© The Authors 2023.Context. The Transiting Exoplanet Survey Satellite (TESS) mission has provided ph...
The characterization of exoplanets conditions cannot be based solely on the knowlegde of the planeta...
The study of stellar oscillations - asteroseismology - has revolutionized our understanding of the p...
The Transiting Exoplanet Survey Satellite (TESS) is a NASA Astrophysics Explorer mission. Following ...
It is well known that asteroseismology is the unique technique permitting the study of the internal ...
Studying the internal structure of exoplanet-host stars compared to that of similar stars without de...