Abundances in Very Metal-Poor Stars

Simple item page
dc.creatorRyan, Sean G.
dc.date2000-01-13
dc.date.accessioned2026-07-07T01:51:43Z
dc.date.available2026-07-07T01:51:43Z
dc.descriptionMetal-poor stars provide information on the characteristics and chemical evolution of the halo population of the Galaxy, the first epoch of star formation and Galaxy formation (not just locally but with relevance to high-redshift objects), and big bang nucleosynthesis. This review looks at recent developments in this subject.
dc.descriptionProc. 35th Liege International Astrophysics Colloquium, Liege, 1999 "The Galactic Halo: From Globular Clusters to Field Stars" A. Noels, P. Magain, D. Caro, E. Jehin, G. Parmentier, & A. Thoul (eds) 16 pages including 7 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0001235
dc.identifierhttp://arxiv.org/abs/astro-ph/0001235
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/390
dc.subjectAstrophysics
dc.titleAbundances in Very Metal-Poor Stars
dc.typetext

Files

Collections

arXiv