arXiv (All)
open access
The H IX galaxy survey IV: What does the molecular gas reveal in HI eXtreme galaxies
Galaxies with extreme amounts of neutral atomic hydrogen (HI), known as HI-eXtreme (HIX) galaxies, paradoxically exhibit normal or low star formation rates. To investigate the bottleneck in their star formation, we present ALMA CO(1-0) observations for five HIX survey galaxies: ESO208-G026, ESO378-G
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
- ALMA Chemical Evolution (ACE) Survey: Molecular gas properties of low-mass, low-metallicity galaxies at cosmic noon#1035042
- Chemical and dynamical evolution in gas-rich dwarf galaxies#639540
- A Sample of 459 Galaxy Groups Identified from the FAST All Sky HI Survey DR2#1050246
- WALLABY pilot survey: accurate and automated linewidth measurements from global HI profiles#1327647
- Ionized Gas Kinematics and Star-forming Clumps in Extremely Metal-poor Galaxies#1402589
Record · ID 1413211
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