arXiv (OAI Expanded)
open access
On radial gas flows, the Galactic Bar and chemical evolution in the Galactic Disc
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
- Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N#1123153
- ALMA Chemical Evolution (ACE) Survey: Molecular gas properties of low-mass, low-metallicity galaxies at cosmic noon#1035042
- Chemical evolution of the Milky Way disc with radial gas flows: a Lagrangian approach#1109091
- Bower Reservoir Relation: Newtonian Disk Structure Predicts the Residual Speed Gas Fraction Trend in Disk Galaxies#478478
- The role of outflows and star formation efficiency in the evolution of early-type cluster galaxies#639550
Record · ID 639471
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