arXiv (All)
open access
Multiplicity of Massive stars in the Milky Way (M3W). II. The brightest single O stars: variability and systemic velocities
(ABRIDGED) M3W studies the dynamical properties of massive stars in the solar vicinity, such as their systemic velocities, which are affected by variability effects: pulsations, line infilling by wind and disks, and incomplete knowledge about the central wavelengths. We want to increase the accuracy
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
- CADIS deep star counts: Galactic structure and the stellar luminosity function#639344
- Fundamental parameters of Galactic luminous OB stars V. The effect of microturbulence#639587
- Radiation Pressure Instability-Driven Variability of Line-Driven Disk Winds in AGNs: Connection to Periodic Luminosity Variations and UFO Appearance#1122653
- Constraints on the Intranight Optical Variability of Intermediate-Mass Black Hole Candidates#822575
- Molecular atlas of nearby galaxies through sensitive high-resolution multi-band molecular line surveys#1357342
Record · ID 1458063
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