Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-20T17:29:53.081Z Has data issue: false hasContentIssue false
  • English
  • Français

Abundance Ratios in Barium Stars

Published online by Cambridge University Press:  23 December 2005

D.M. Allen  and
B. Barbuy
D.M. Allen
Affiliation:
IAG-USP, Rua do Matão 1226, São Paulo, 05508-900, Brazil email: [email protected]
B. Barbuy
Affiliation:
IAG-USP, Rua do Matão 1226, São Paulo, 05508-900, Brazil email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

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.

Abundances of α-, iron peak, s- and r-elements were determined for a sample of Barium stars and the [α,iron peak/s], [α,iron peak/r], [s/r] ratios were derived.

Keywords

Stars: abundancesstars: AGB and post-AGBnuclear reactionsnucleosynthesisabundance
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S228: From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution , May 2005 , pp. 479 - 480
Copyright
© 2005 International Astronomical Union