Asteroseismology of Solar-Type and Red-Giant Stars

Abstract

We are entering a golden era for stellar physics driven by satellite and telescope observations of unprecedented quality and scope. New insights on stellar evolution and stellar interiors physics are being made possible by asteroseismology, the study of stars by the observation of natural, resonant oscillations. Asteroseismology is proving to be particularly significant for the study of solar-type and red-giant stars. These stars show rich spectra of solar-like oscillations, which are excited and intrinsically damped by turbulence in the outermost layers of the convective envelopes. In this review we discuss the current state of the field, with a particular emphasis on recent advances provided by the Kepler and CoRoT space missions and the wider significance to astronomy of the results from asteroseismology, such as stellar populations studies and exoplanet studies.

The following paper will appear in the 2013 volume of Annual Reviews of Astronomy and Astrophysics (88 pages, 7 figures; references updated; further corrections to typos during galley-proof review)

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• Lessons learnt from the Solar neighbourhood and the Kepler field
• Applying Vision Transformers on Spectral Analysis of Astronomical Objects
• The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• Comprehensive Parameter Determination of Exoplanet through Asteroseismic Host Star Constraints
• Prelude to, and Nature of the Space Photometry Revolution
• Advanced asteroseismic modelling: breaking the degeneracy between stellar mass and initial helium abundance
• Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
• Excitation and Damping of Oscillation Modes in Gaseous Planets
• Chromospheric emission of solar-type stars with asteroseismic ages
• Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
• Hidden oscillations in plain sight: identification of seismically unresolved red-giant asteroseismic binary candidates
• The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
• The SAGA so far: reading the history of the Galaxy with asteroseismology
• Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra
• Spectroscopic constraints for low-mass asteroseismic targets