Skip to main content

O and α-Element Abundances in Metal-Poor Stars

  • Conference paper
  • 64 Accesses

Abstract

Since about thirty years it is known that Oxygen and other α—elements are overabundant in metal-poor stars. In this talk I briefly review the historical and theoretical background, discuss reliability of present abundance determinations for O, and finally comment about the implications relevant to galactic chemical evolution.

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1999 Springer Science+Business Media Dordrecht

About this paper

Cite this paper

Gratton, R.G. (1999). O and α-Element Abundances in Metal-Poor Stars. In: Spite, M. (eds) Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4213-7_25

Download citation

  • DOI: https://doi.org/10.1007/978-94-011-4213-7_25

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5831-5

  • Online ISBN: 978-94-011-4213-7

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics