Article contents
Chemically tagging the Galactic disk: abundance patterns of old open clusters
Published online by Cambridge University Press: 01 June 2008
Abstract
The long term goal of large-scale chemical tagging is to use stellar elemental abundances as a tracer of dispersed substructures of the Galactic disk. The identification of such lost stellar aggregates and exploring their chemical properties will be key in understanding the formation and evolution of the disk. Present day stellar structures such as open clusters and moving groups are the ideal testing grounds for the viability of chemical tagging, as they are believed to be the remnants of the original larger star-forming aggregates. We examine recent high resolution abundance studies of open clusters to explore the various abundance trends and reassess the prospects of large-scale chemical tagging.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Issue S254: The Galaxy Disk in Cosmological Context , June 2008 , pp. 133 - 138
- Copyright
- Copyright © International Astronomical Union 2009
References
- 1
- Cited by