Correlated Strontium and Barium Isotopic Compositions of Acid-Cleaned Single Silicon Carbides from Murchison
arXiv:1501.05883 · doi:10.1088/0004-637X/803/1/12
Abstract
We present strontium, barium, carbon, and silicon isotopic compositions of 61 acid-cleaned presolar SiC grains from Murchison. Comparison with previous data shows that acid washing is highly effective in removing both strontium and barium contamination. For the first time, by using correlated / and / ratios in mainstream SiC grains, we are able to resolve the effect of concentration from that of -pocket mass on s-process nucleosynthesis, which points towards the existence of large -pockets with low concentration in AGB stars. The presence of such large R-pockets with a variety of relatively low concentrations seems to require multiple mixing processes in parent AGB stars of mainstream SiC grains.
References in corpus (4)
- Galactic Chemical Evolution and solar s-process abundances: dependence on the 13C-pocket structure
- Barium Isotopic Composition of Mainstream Silicon Carbides from Murchison: Constraints for s-Process Nucleosynthesis in AGB Stars
- Heavy elements in Globular Clusters: the role of AGB stars
- The 13C-Pocket Structure in AGB Models: Constraints from Zirconium Isotope Abundances in Single Mainstream SiC Grains
Cited by in corpus (23)
- Magnetic-buoyancy Induced Mixing in AGB Stars: Presolar SiC Grains
- The s Process and Beyond
- Galactic Chemical Evolution: the Impact of the 13C-pocket Structure on the s-process Distribution
- Re-evaluation of the Ne()Mg and Ne()Mg reaction rates
- Constraints of the physics of low-mass AGB stars from CH and CEMP stars
- Horizons: Nuclear Astrophysics in the 2020s and Beyond
- s-Processing in AGB Stars Revisited. III. Neutron captures from MHD mixing at different metallicities and observational constraints
- Presolar grain isotopic ratios as constraints to nuclear and stellar parameters of AGB nucleosynthesis
- J-type carbon stars: A dominant source of 14N-rich presolar SiC grains of type AB
- Origin of large meteoritic SiC stardust grains in metal-rich AGB stars
- s-Processing from MHD-induced mixing and isotopic abundances in presolar SiC grains
- Partial mixing and the formation of 13C pockets in AGB stars: effects on the s-process elements
- On the mass and metallicity distribution of parent AGB stars of presolar SiC
- New Multielement Isotopic Compositions of Presolar SiC Grains: Implications for Their Stellar Origins
- Slow Neutron-Capture Process: Low-mass AGB stars and presolar silicon carbide grains
- Presolar Silicon Carbide Grains of Types Y and Z: Their Strontium and Barium Isotopic Compositions and Stellar Origins
- Presolar grains
- The NuGrid AGB Evolution and Nucleosynthesis Data Set
- Representation of s-process abundances for comparison to data from bulk meteorites
- Impact of - and -dependent decay rates and new (n,) cross sections on the process in low-mass AGB stars
- Strontium-84 Enrichments in Presolar Grains Provide First Evidence of p-process Nucleosynthesis in Core-collapse Supernovae
- Modeling the formation of the C neutron source in AGB stars
- Production of n-rich nuclei in red giant stars