arXiv · astro-ph/0101561
Galactic Chemical Evolution and the abundances of lithium, beryllium and boron
Abstract
A LiBeB evolution model including Galactic Cosmic Ray nucleosynthesis, the $ν$-process, novae, AGB and C-stars is presented. We have included Galactic Cosmic Ray Nucleosynthesis (GCRN) in a complete Chemical Evolution Model that takes into account 76 stable isotopes from hydrogen to zinc. Any successful LiBeB evolution model should also be compatible with other observational constraints like the age-metallicity relation, the G-dwarf distribution or the evolution of other elements. At the same time, we have checked how different would be a model that took into account the last observations by Wakker et al. (1999) of metal-enriched clouds falling onto the disk, from a primordial infall model.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Andreu Alibes, Javier Labay, Ramon Canal. 2001-01-31. Galactic Chemical Evolution and the abundances of lithium, beryllium and boron. https://doi.org/10.1142/9789812810830_0030
Cite the original work for its findings. Save a collection to share your selection of sources.