Extremely metal-poor stars: the need for UV spectra
by Piercarlo Bonifacio, Elisabetta Caffau, and Monique Spite
Published onMay 31, 2019
Extremely metal-poor stars: the need for UV spectra
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Abstract
Extremely metal-poor stars are the fossil record of the gas in the pristine Universe. They offer us the opportunity to understand the mass distribution and nucleosynthetic properties of the First generation of stars. UV spectra provide access to information not available in other spectral ranges.
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