Abstract
The CoRoT and Kepler space missions have detected oscillations in hundreds of Sun-like stars and thousands of field red-giant stars. This has opened the door to a new era of stellar population studies in the Milky Way. We report on the current status and future prospects of harvesting space-based photometric data for ensemble asteroseismology, and highlight some of the challenges that need to be faced to use these stars as accurate clocks and rulers for Galactic studies.
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We assume an extension of the overshooting region equal to 0. 2 H p , where H p is the pressure scale height at the boundary of the convective core, as defined by the Schwarzschild criterion.
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Miglio, A., Girardi, L., Rodrigues, T.S., Stello, D., Chaplin, W.J. (2015). Solar-Like Oscillating Stars as Standard Clocks and Rulers for Galactic Studies. In: Miglio, A., Eggenberger, P., Girardi, L., Montalbán, J. (eds) Asteroseismology of Stellar Populations in the Milky Way. Astrophysics and Space Science Proceedings, vol 39. Springer, Cham. https://doi.org/10.1007/978-3-319-10993-0_2
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