Extremely metal-poor stars: the need for UV spectra - Observatoire de Paris
Article Dans Une Revue Bulletin of the American Astronomical Society Année : 2019

Extremely metal-poor stars: the need for UV spectra

Résumé

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.

Dates et versions

obspm-04009798 , version 1 (01-03-2023)

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Piercarlo Bonifacio, Elisabetta Caffau, Monique Spite. Extremely metal-poor stars: the need for UV spectra. Bulletin of the American Astronomical Society, 2019, 51, ⟨10.48550/arXiv.1903.05666⟩. ⟨obspm-04009798⟩
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