arXiv (All)
open access
Stellar Collisions from Self-consistent Stellar Dynamics Around Growing Supermassive black Holes
The centers of galaxies harbor the densest stellar environments, where a massive black hole (MBH) accelerates stars to such high velocities that direct collisions can result in high-energetic phenomena, such as gravitational wave sources, kilonovae, and supernova-like transients. These collisions ca
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
- Formation of black hole stars via star--black hole collisions#780902
- Formation of black hole stars via star--black hole collisions#779527
- Thermal and non-thermal emission from supermassive black hole circumbinary disks: Disks, Coronae, Streams, and Cavities#925503
- Potential binary supermassive black holes in Markarian 231 as a scientific case for the spectropolarimeter POLLUX#1077405
- Self-interacting dark matter delays bar growth in an isolated gas-rich galactic disk: torque-resolved numerical evidence#1012531
Record · ID 1077065
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