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.

Dates and versions

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

Identifiers

Cite

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⟩
11 View
0 Download

Altmetric

Share

More