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- W1637636641 abstract "We are now seeing a new generation of stellar models based on the recent opacity tables by Rogers and Iglesias (1992). Various changes in other important physical ingredients like nuclear reaction rates, convection parameters, mass loss rates, helium/metal ratios, relative abundances of heavy elements etc. are also included. Besides the Sun the most obvious objects for confrontation of the new grids with observations are binary components, pulsating stars, and well-studied open and globular clusters. Among these candidates the detached, double-lined eclipsing binaries play a unique role as our only source of absolute dimensions which 1) can be considered valid for single stars and 2) are accurate enough for serious tests of the input physics of modern stellar models." @default.
- W1637636641 created "2016-06-24" @default.
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- W1637636641 date "1993-01-01" @default.
- W1637636641 modified "2023-09-25" @default.
- W1637636641 title "[Fe/H] and lithium Abundance for Detached Eclipsing Binaries" @default.
- W1637636641 cites W2014244408 @default.
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- W1637636641 doi "https://doi.org/10.1017/s0252921100017711" @default.
- W1637636641 hasPublicationYear "1993" @default.
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