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Inverse Problems in Asteroseismology
Published 20 Aug 2018 in astro-ph.SR and cs.LG | (1808.06649v1)
Abstract: Asteroseismology allows us to probe the internal structure of stars through their global modes of oscillation. Thanks to missions such as the NASA Kepler space observatory, we now have high-quality asteroseismic data for nearly 100 solar-type stars. In this thesis, new techniques to measure the ages, masses, and radii of stars are presented, as well as a way to infer their internal structure.
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