Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2025-01-02T17:55:33.032Z Has data issue: false hasContentIssue false
  • English
  • Français

Lithium in population II stars

Published online by Cambridge University Press:  07 August 2017

F. Spite ,
M. Spite ,
R. Cayrel  and
S. Huille
F. Spite
Affiliation:
Observatoire de Paris 92195 Meudon Cedex France
M. Spite
Affiliation:
Observatoire de Paris 92195 Meudon Cedex France
R. Cayrel
Affiliation:
Observatoire de Paris 92195 Meudon Cedex France
S. Huille
Affiliation:
Observatoire de Paris 92195 Meudon Cedex France

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

NEW data about dwarfs: a few more metal-poor dwarfs have been observed for lithium at the CAT + CES at La Silla (ESO). These new results, together with a few new measurements in the literature show again a constant lithium abundance, confirming the trend previously found (the plateau). Let us note however that two metal-poor dwarfs have recently been reported with a low lithium abundance. Obviously, more observations are needed.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 490
Copyright
Copyright © Kluwer