No CrossRef data available.
Article contents
Binarity in CEMP-no stars
Published online by Cambridge University Press: 02 August 2018
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 monitor a sample of CEMP-no stars using the CFHT and SALT telescopes to gain additional knowledge about the possible binarity of these stars. This information is valuable for each individual star, and additionally it could be used to further constrain their binary fraction. We find two new CEMP-no binaries and four additional CEMP-no stars that show some indication of radial velocity variations, resulting in a CEMP-no binary fraction of ~20%.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 273 - 274
- Copyright
- Copyright © International Astronomical Union 2018
References
Starkenburg, E., Shetrone, M. D., McConnachie, A. W., & Venn, K. A., 2014, MNRAS, 441, 1217Google Scholar
You have
Access