Lower Limits on the Nucleosynthesis of 44Ti and 60Fe in the Dynamic Spiral-arm Cosmic-Ray Propagation Model
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/863/i=1/a=86/pdf
Reference42 articles.
1. Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
2. RECOVERING THE OBSERVED B/C RATIO IN A DYNAMIC SPIRAL-ARMED COSMIC RAY MODEL
3. THE B/C AND SUB-IRON/IRON COSMIC RAY RATIOS—FURTHER EVIDENCE IN FAVOR OF THE SPIRAL-ARM DIFFUSION MODEL
4. Electron-capture Isotopes Could Constrain Cosmic-Ray Propagation Models
5. Observation of the 60 Fe nucleosynthesis-clock isotope in galactic cosmic rays
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1. Reaction Rate Sensitivity of the Production of γ-Ray Emitting Isotopes in Core-collapse Supernovae;The Astrophysical Journal;2020-09-01
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