eScholarship
metadata only
Branching Ratios in Vacuum Ultraviolet Photodissociation of CO and N2: Implications for Oxygen and Nitrogen Isotopic Compositions of the Solar Nebula
NASA’s Genesis mission reveals that the rare isotope 15N is approximately seven times more enriched than the rare isotopes 17O and 18O in the terrestrial planets relative to the Sun. Here, we explain this peculiar observation under the framework of self-shielding and the difference in chemical react
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
- JWST observations of photodissociation regions. I. Aliphatic and aromatic carbonaceous dust, ices, and gas-phase spectral line inventory#314984
- Tracing the Hidden Molecular Gas in the Small Magellanic Cloud with SOFIA and APEX#972731
- CECILIA: Multi-line Constraints on Excess Nebular Emission from Low-Ionization Gas at Cosmic Noon#1063292
- Exploring the observed properties of JWST Little Red Dots with cosmological simulations and dust radiative transfer#1129514
- Unified modelling of broad and narrow optical-UV emission lines from massive black holes: interpreting high-redshift JWST observations#1000035
Record · ID 1263369
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