arXiv (All)
open access
$^{16}$O(p,$γ$)$^{17}$F Reaction and the C and O Isotopic Ratios in Red Giant Branch Stars
The $^{16}$O/$^{17}$O isotopic ratio is a widely used tracer of nucleosynthesis and mixing processes in red giant stars. Its value depends on the rates of the proton-capture reactions responsible for the production and destruction of $^{16}$O and $^{17}$O among which the $^{16}$O(p,$γ$)$^{17}$F reac
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- $^{12}$C + $^{17}$O reaction#652900
- Search for massive WH resonances decaying into the ℓνbb¯ final state at s=8TeV#1328461
- $S$ factor of $^{13}$C($α$,$n$)$^{16}$O at low energies in cluster effective field theory#1326220
- 12 CFR Part 237 — Swaps Margin and Swaps Push-out (Regulation KK)#505326
- Proton-Induced Deuteron Knockout (p,pd) on $^{12}$C and $^{16}$O at 226 MeV#231673
Record · ID 1355166
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive