Extremely metal-poor stars: the need for UV spectra - Observatoire de Paris
Journal Articles Bulletin of the American Astronomical Society Year : 2019

Extremely metal-poor stars: the need for UV spectra

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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Sciences of the Universe [physics]

Isabelle Guinouard  : Connect in order to contact the contributor

https://hal-obspm.ccsd.cnrs.fr/obspm-04009798

Submitted on : Wednesday, March 1, 2023-1:50:41 PM

Last modification on : Friday, April 19, 2024-4:19:00 PM

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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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