Finger on the pulse of asteroseismology
arXiv:2306.15070 · doi:10.1093/astrogeo/atad007
Abstract
Warrick Ball highlights some recent discoveries in the context of the past, present and future of asteroseismology.
Author-produced version of article accepted in Astronomy & Geophysics
References in corpus (17)
- A new asteroseismic diagnostic for internal rotation in Doradus stars
- Very regular high-frequency pulsation modes in young intermediate-mass stars
- A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS
- 30 to 100-kG magnetic fields in the cores of red giant stars
- Age dating of an early Milky Way merger via asteroseismology of the naked-eye star Indi
- Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades
- Blue large-amplitude pulsators as a new class of variable stars
- Dipole modes with depressed amplitudes in red giants are mixed modes
- First evidence of inertial modes in Doradus stars: The core rotation revealed
- A precise asteroseismic age and metallicity for HD 139614: a pre-main-sequence star with a protoplanetary disc in Upper-Centaurus Lupus
- The single-sided pulsator CO~Camelopardalis
- A Catalogue of Solar-Like Oscillators Observed by TESS in 120-second and 20-second Cadence
- Tess asteroseismology of the known planet host star Fornacis
- Five young Scuti stars in the Pleiades seen with Kepler/K2
- Oscillations in the Sun with SONG: Setting the scale for asteroseismic investigations
- Robust asteroseismic properties of the bright planet host HD 38529
- A Distant Mirror: Solar Oscillations Observed on Neptune by the Kepler K2 Mission