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- W1569470627 abstract "The five-year goal of this effort is to calculate high fidelity mid-W spectra for individual stars and stellar systems for a wide range of ages, abundances, and abundance ratios. In this second year, the comparison of our calculations against observed high-resolution mid- W spectra was extended to stars as metal-rich as the Sun, and to hotter and cooler stars, further improving the list of atomic line parameters used in the calculations. We also published the application of our calculations based on the earlier list of line parameters to the observed mid-UV and optical spectra of a mildly metal-poor globular cluster in the nearby Andromeda galaxy, Messier 3 1." @default.
- W1569470627 created "2016-06-24" @default.
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- W1569470627 date "2003-01-05" @default.
- W1569470627 modified "2023-09-23" @default.
- W1569470627 title "Comparing Ultraviolet Spectra Against Calculations: First Results" @default.
- W1569470627 hasPublicationYear "2003" @default.
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