arXiv (All)
open access
The coupled evolution of nuclear star clusters and intermediate-mass black holes in a dwarf-galaxy merger
Nuclear star clusters (NSCs) and intermediate-mass black holes (IMBHs) are expected to coexist in low-mass galaxies and might together facilitate the coalescence and growth of IMBHs. We simulate an equal-mass, gas-rich dwarf-galaxy merger in which each progenitor hosts a $10^3\,\rm M_\odot$ IMBH emb
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
- TNGC-SIDM I: Evolution of massive cluster mergers under the self-interacting dark matter paradigm#1344780
- Exemplary Merging Clusters II: XMM-Newton and Chandra X-ray Observations of MACS J1752.0+4440 and ZwCl 1856.8+6616#1247607
- The Birth and Early Feedback of Massive Star Clusters Across the Local Universe#1356548
- Could merged star-clusters build up a small galaxy?#639333
- Pushing Variability Searches to Extreme Dwarf Galaxies with the Vera C. Rubin Observatory Data Preview 2#1247682
Record · ID 1489837
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