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• W3101447520 abstract "Red-giant stars are low- to intermediate-mass ($M lesssim 10$~M$_{odot}$) stars that have exhausted hydrogen in the core. These extended, cool and hence red stars are key targets for stellar evolution studies as well as galactic studies for several reasons: a) many stars go through a red-giant phase; b) red giants are intrinsically bright; c) large stellar internal structure changes as well as changes in surface chemical abundances take place over relatively short time; d) red-giant stars exhibit global intrinsic oscillations. Due to their large number and intrinsic brightness it is possible to observe many of these stars up to large distances. Furthermore, the global intrinsic oscillations provide a means to discern red-giant stars in the pre-helium core burning from the ones in the helium core burning phase and provide an estimate of stellar ages, a key ingredient for galactic studies. In this lecture I will first discuss some physical phenomena that play a role in red-giant stars and several phases of red-giant evolution. Then, I will provide some details about asteroseismology -- the study of the internal structure of stars through their intrinsic oscillations -- of red-giant stars. I will conclude by discussing galactic archaeology -- the study of the formation and evolution of the Milky Way by reconstructing its past from its current constituents -- and the role red-giant stars can play in that." @default.
• W3101447520 created "2020-11-23" @default.
• W3101447520 creator A5074798637 @default.
• W3101447520 date "2017-07-06" @default.
• W3101447520 modified "2023-09-27" @default.
• W3101447520 title "Asteroseismology of Red Giants and Galactic Archaeology" @default.
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• W3101447520 doi "https://doi.org/10.1007/978-3-319-59315-9_5" @default.
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