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- W2079220532 abstract "Abstract The distances to old stellar populations have traditionally been derived from three standard candles: the luminosity of the red-giant-branch tip, the absolute magnitudes of RR Lyrae stars, and the colour–magnitude-diagram loci of nearby subdwarfs. The distance-modulus uncertainties that are associated with these methods are still at the level of ±0.10–0.15 mag. Current stellar models are able to satisfy these age-independent constraints to well within their error bars, which are mainly owing to the uncertainties in the distances of the calibrating objects and, directly or indirectly, to chemical-abundance uncertainties. The impact of varying the physics and the assumed abundances in stellar models on the aforementioned standard candles is discussed, as is the use of the giant-branch bump luminosity to constrain the distance scale." @default.
- W2079220532 created "2016-06-24" @default.
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- W2079220532 date "2012-08-01" @default.
- W2079220532 modified "2023-09-26" @default.
- W2079220532 title "The effects of physics and chemical-abundance uncertainties on the properties of lower-mass stars that are used as standard candles" @default.
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- W2079220532 doi "https://doi.org/10.1017/s1743921312021308" @default.
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