No CrossRef data available.
Article contents
Non-equilibrium Dynamical Processes in the Galaxy
Published online by Cambridge University Press: 21 October 2010
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.
Dynamical models have often necessarily assumed that the Galaxy is nearly steady state or dynamically relaxed. However observed structure in the stellar metallicity, spatial and velocity distributions imply that heating, mixing and radial migration has taken place. Better comprehension of non-equilibrium processes will allow us to not only better understand the current structure of the galaxy but its past evolution.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 178 - 179
- Copyright
- Copyright © International Astronomical Union 2010
References
Minchev, I., Boily, C., Siebert, A., & Bienayme, O. 2009, submitted to MNRAS, arXiv0909.3516Google Scholar
Minchev, I., Quillen, A. C., Williams, M., Freeman, K. C., Nordhaus, J., Siebert, A., & Bienaymé, O. 2009, MNRAS, 396, L56CrossRefGoogle Scholar
Quillen, A. C., Minchev, I., Bland-Hawthorn, J., & Haywood, M. 2009, MNRAS, 397, 1599CrossRefGoogle Scholar
You have
Access