Probing the interior physics of stars through asteroseismology
arXiv:1912.12300 · doi:10.1103/RevModPhys.93.015001
Abstract
Yearslong time series of high-precision brightness measurements have been assembled for thousands of stars with telescopes operating in space. Such data have allowed astronomers to measure the physics of stellar interiors via nonradial oscillations, opening a new avenue to study the stars in the Universe. Asteroseismology, the interpretation of the characteristics of oscillation modes in terms of the physical properties of the stellar interior, brought entirely new insights in how stars rotate and how they build up their chemistry throughout their evolution. Data-driven space asteroseismology delivered a drastic increase in the reliability of computer models mimicking the evolution of stars born with a variety of masses and metallicities. Such models are critical ingredients for modern physics as a whole, because they are used throughout various contemporary and multidisciplinary research fields in space science, including the search for life outside the solar system, archaeological studies of the Milky Way, and the study of single and binary supernova progenitors, among which are future gravitational wave sources. The specific role and potential of asteroseismology for those modern research fields are illustrated. The review concludes with current limitations of asteroseismology and highlights how they can be overcome with ongoing and future large infrastructures for survey astronomy combined with new theoretical research in the era of high-performance computing. This review presents results obtained through major community efforts over the past decade. These breakthroughs were achieved in a collaborative and inclusive spirit that is characteristic of the asteroseismology community. The review's aim is to make this research field accessible to graduate students and readers coming from other fields of physics, with incentives to join future applications in this domain of astrophysics.
69 pages, 1 table, 19 figures (downgraded in resolution to meet the arXiv limits). Accepted for publication in Reviews of Modern Physics. Author's version based on a proof prepared by the publisher (Journal publication is foreseen in March 2021)
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- Asteroseismic modelling of main-sequence solar-like stars and Kepler exoplanet host stars with the FICO procedure I. Catalogue of fundamental stellar properties
- Discovery of Sct Components in Eclipsing Binary Systems IQ CMa, AW Men and W Vol
- Asteroseismic detection of an internal magnetic field in the B0.5V pulsator HD 192575
- KIC 10855535: An elegant Delta Scuti pulsator with Amplitude and Phase Modulation
- Dynamics of azimuthal thermoacoustic modes in imperfectly symmetric annular geometries
- KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern
- Characterizing bright Scuti pulsators using TESS lightcurves
- Asteroseismology of sz lyn using multi-band high time resolution photometry from ground and space
- Exploring the unexpected: Disharmonized harmonic pulsation modes in high-amplitude Scuti stars
- Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission
- Nuclear astrophysics
- Probing the internal magnetism of stars using asymptotic magneto-asteroseismology
- Eclipse mapping study of the eclipsing binary KIC~3858884 with hybrid ~Sct/~Dor component
- Matching seismic masses for RR Lyrae-type and oscillating red horizontal-branch stars in M4
- Asteroseismology
- A self-consistent numerical model of internal wave-induced mean flow oscillations in polar geometry
- Automated all-sky detection of γ Doradus / δ Scuti hybrids in TESS data from positive unlabelled (PU) learning
- PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators
- Exploring Late Stellar Evolution in the Era of Large Surveys: Machine Learning Prospects for Hot Subdwarfs and White Dwarfs
- KIC 3868420: A high-amplitude Scuti- Dor hybrid star crossing the Hertzsprung gap
- Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
- Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images
- Perspectives on the Physics of Late-Type Stars from Beyond Low Earth Orbit, the Moon and Mars
- Orbital and Pulsation Analysis of 42 Heartbeat Stars Discovered in TESS Data
- Predicting Stellar Parameters of Massive Stars from Light Curves with Machine Learning
- Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
- Harmonics as a Hidden Window into the Turbulent Convective Envelope of non-Blazhko RRab Stars
- Zeta-Payne: a fully automated spectrum analysis algorithm for the Milky Way Mapper program of the SDSS-V survey
- The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
- One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations
- Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2
- New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
- A summary of instruments proposed for observing pulsating variables from the Mt. Abu Observatory
- Fast optical variability in Supergiant X-ray binaries
- Asteroseismic Analysis of a Red Giant KIC 9145955 by Including the Small-scale Magnetic Fields in the Atmosphere
- A magnetic field detection in the massive O-type bright giant 63 Oph
- Amplitude and frequency modulation of super-Nyquist frequency from Kepler photometric sampling
- The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry