arXiv (All)
open access
Precise physical and kinematical parameters of massive eclipsing binaries in the Small Magellanic Cloud
The formation of massive stars serves an important field of study, requiring research into whether these stars need to form together within clusters of low-mass stars or if they are able to form independently. Currently, there has been an increase in the number of massive stars found far from cluste
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
- Hubble Space Telescope survey of Magellanic Cloud star clusters. Binaries, mass functions, blue stragglers, and structural parameters#355523
- The dispersal law of young star clusters: free expansion -- A Gaia/eROSITA census of Orion and Sco--Cen#972124
- The VISCACHA survey - X. A fast method to build completeness maps for Magellanic Clouds star clusters 10#270290
- The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-Day Location#1110555
- FEAST: Probing Hierarchical Star Formation with the Spatial Distributions of Young Star Clusters#215471
Record · ID 984761
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