arXiv (All)
open access
Examining Turbulence in Galactic Molecular Clouds. II. Turbulence Cascade Beyond the Scale of Giant Molecular Clouds
We use $^{12}$CO (J=1--0) data from the MWISP survey to investigate turbulence in a $\sim$kpc-scale segment of the Local Arm. By slicing the position-position-velocity cube into narrow layers that follow the Galactic-rotation trend in the $L$-$V$ diagram, we find that the structure functions (SFs) a
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
- Dynamic Spacetime Fluid Theory (FED 2.5): A Consistent Framework for Fractal Density Networks and Galactic Rotation Curves. Consolidated and Verified Version.#118962
- Unifying Galactic Dynamics and Cluster Collisions via a Phase-Transitioning Vacuum Fluid#187077
- Gravitational Resonance Linking: A Complete Framework for Galactic Dynamics#30018
- NGC 1901: A new benchmark cluster for gyrochronology in the TESS Southern continuous viewing zone#925653
- Dynamical Activation of a Transition Scale in Galactic Rotation Curves#176250
Record · ID 987503
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