Concluding remarks
arXiv:astro-ph/0612056 · doi:10.1017/S1743921307001056
Abstract
To be published in the proceedings of IAU Symposium 239 "Convection in Astrophysics" (ed. F. Kupka, I. W. Roxburgh, K. L. Chan). Content: 1. From Nice to Prague, 2. The triumph of 3-D simulations, 3. How to lower the cost - what else can be done? 4. A powerful tool to determine surface abundances, 5. The effects of convection are not confined to convection zones, 6. Towards a realistic model of the solar dynamo, 7. The moment of truth: facing observational tests, 8. On my wish-list.
arXiv comment6 pages
References in corpus (4)
- Influence of gravity waves on the internal rotation and Li abundance of solar-type stars
- The large-scale axisymmetric magnetic topology of avery-low-mass fully-convective star
- Dynamo Action in the Solar Convection Zone and Tachocline: Pumping and Organization of Toroidal Fields
- Simulations of core convection in rotating A-type stars: Magnetic dynamo action