arXiv (All)
open access
The Tilt of the Velocity Ellipsoid in the Milky Way Disk with GALAH-Gaia Data
We investigate the metallicity dependence of the tilt of the velocity ellipsoid using more than 572,000 stars selected from GALAH and Gaia. We find that the tilt angles of disk stars can be well described by the relation $α= α_{0}\,\mathrm{arctan}(Z/R)$, and the $α_{0}$ differ significantly among di
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
- HD 120678: a classical Be star with a tilting heartbeat disk#1355191
- Internal Structure, Not Environment, Shapes Metallicity Gradients in Low-Mass Galaxies from MaNGA#1144656
- New Optical and Mid-Infrared RR Lyrae Period-Luminosity-Metallicity Relations for Precision Distances and Metallicity Distributions in the Magellanic Clouds#1063330
- The IBISCO survey: I. Multiphase discs and winds in the Seyfert galaxy Markarian 509#1166624
- DIISC-VII: Linking Radial Gas Motions to Anomalously Low Metallicity Star-forming Regions in the XUV Disk of NGC 3344#1063095
Record · ID 1326599
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