TESS Asteroseismology of the Known Red-giant Host Stars HD 212771 and HD 203949
The Transiting Exoplanet Survey Satellite (TESS) is performing a near all-sky survey for planets that transit bright stars. In addition, its excellent photometric precision enables asteroseismology of solar-type and red-giant stars, which exhibit convection-driven, solar-like oscillations. Simulations predict that TESS will detect solar-like
Campante, Tiago L. et al.
Fecha de publicación:
11
2019