2019•arXiv (Cornell University)Open access
Astro2020 Science White Paper: gravity-wave asteroseismology of intermediate- and high-mass stars
A. Tkachenko, C. Aerts, D. M. Bowman, T. Van Reeth, J. De Ridder, C. Johnston, M. G. Pedersen, Siemen Burssens, Mathias Michielsen, Joey S. G. Mombarg, S. Sekaran, R. Björklund, T. M. Rogers, P. V. F. Edelmann, R. P. Ratnasingam, K. Zwintz, Juna A. Kollmeier, Jennifer A. Johnson, Hans-Walter Rix, Jamie Tayar
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Abstract
The evolution of a star is driven by the physical processes in its interior making the theory of stellar structure and evolution the most crucial ingredient for not only stellar evolution studies, but any field of astronomy which relies on the yields along stellar evolution. High-precision time-series photometric data assembled by recent space missions revealed that current models of stellar structure and evolution show major shortcomings already in the two earliest nuclear burning phases, impacting all subsequent phases prior to the formation of the end-of-life remnant. This white paper focuses specifically on the transport of chemical elements and of angular momentum in the stellar structure and evolution models of stars born with convective core, as revealed by their gravity-mode oscillations.
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