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• W3104803313 abstract "Abstract This overview summarizes the age dating methods available for young sub-solar mass stars. Pre-main sequence age diagnostics include the Hertzsprung-Russell (HR) diagram, spectroscopic surface gravity indicators, and lithium depletion; asteroseismology is also showing recent promise. Near and beyond the zero-age main sequence, rotation period or vsin i and activity (coronal and chromospheric) diagnostics along with lithium depletion serve as age proxies. Other authors in this volume present more detail in each of the aforementioned areas. Herein, I focus on pre-main sequence HR diagrams and address the questions: Do empirical young cluster isochrones match theoretical isochrones? Do isochrones predict stellar ages consistent with those derived via other independent techniques? Do the observed apparent luminosity spreads at constant effective temperature correspond to true age spreads? While definitive answers to these questions are not provided, some methods of progression are outlined." @default.
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• W3104803313 date "2008-10-01" @default.
• W3104803313 modified "2023-10-11" @default.
• W3104803313 title "Age-related observations of low mass pre-main and young main sequence stars" @default.
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• W3104803313 doi "https://doi.org/10.1017/s1743921309031731" @default.
• W3104803313 hasPublicationYear "2008" @default.
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