Finger on the pulse of asteroseismology

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)

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• 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
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• Dipole modes with depressed amplitudes in red giants are mixed modes
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• 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 ${\lambda }^2$ Fornacis
• Five young $\delta$ 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