Article contents
Chemical properties of field halo and thick disk blue straggler stars: first results
Published online by Cambridge University Press: 23 December 2005
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.
We have observed with UVES@VLT 15 field Blue Straggler Stars for which kinematical attribution to the Halo or Thick Disk is available. We present here the first results of our detailed chemical analysis.
- Type
- Contributed Papers
- Information
- Copyright
- © 2005 International Astronomical Union
You have
Access
- 1
- Cited by