Barium Isotopic Composition of Mainstream Silicon Carbides from Murchison: Constraints for s-process Nucleosynthesis in Asymptotic Giant Branch Stars.

· by · in , ,

Liu et al. (2014)

The Astrophysical Journal ApJ 786 66. doi:10.1088/0004-637X/786/1/66

LINK

Related posts (automatically generated):

  1. Correlated Strontium and Barium Isotopic Compositions of Acid-cleaned Single Mainstream Silicon Carbides from Murchison
  2. Presolar Grain Isotopic Ratios as Constraints to Nuclear and Stellar Parameters of Asymptotic Giant Branch Star Nucleosynthesis
  3. Slow Neutron-Capture Process: Low-Mass Asymptotic Giant Branch Stars and Presolar Silicon Carbide GrainsOPEN ACCESS 
  4. Do meteoritic silicon carbide grains originate from asymptotic giant branch stars of super-solar metallicity?
  5. Sulfur in presolar silicon carbide grains from asymptotic giant branch stars
  6. Correlated silicon and titanium isotopic compositions of presolar sic grains from the Murchison CM2 chondrite
  7. New Constraints for Supernova Models from Presolar Silicon Carbide X Grains with Very High 26Al/27Al RatiosOPEN ACCESS 
  8. Molybdenum Isotopes in Presolar Silicon Carbide Grains: Details of s-process Nucleosynthesis in Parent Stars and Implications for r- and p-processes
  9. Isotopic study of presolar graphite from the murchison meteorite
  10. NanoSIMS Isotope Studies of Rare Types of Presolar Silicon Carbide Grains from the Murchison Meteorite: Implications for Supernova Models and the Role of 14C
Tags: , , , , , , , , , , , ,