The reaction rate for the destruction of fluorine in AGB stars
✍ Scribed by C. Ugalde; R. Azuma; A. Couture; J. Görres; M. Heil; K. Scheller; E. Stech; W. Tan; M. Wiescher
- Publisher
- Elsevier Science
- Year
- 2005
- Tongue
- English
- Weight
- 193 KB
- Volume
- 758
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
We study how the production of the neutron-rich magnesium isotopes in intermediate mass Asymptotic Giant Branch stars is affected by uncertainties in the neutron-capture reactions involving the Mg isotopes and uncertainties in the 22 Ne + α-capture reaction rates. We also examine how uncertainties i
We propose that the large, radius of $10 3 AU, circumbinary rotating disks observed around some post-asymptotic giant branch (post-AGB) binary stars are formed from slow AGB wind material that is pushed back to the center of the nebula by wide jets. We perform 2D-axisymmetrical numerical simulations