arXiv (All)
open access
Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots
astrophysics-of-galaxiescosmology-and-nongalactic-astrophysicshigh-energy-astrophysical-phenomenasolar-and-stellar-astrophysics
Using gravitational $N$-body simulations, we investigate the evolution of mass and spin for very massive stars (VMSs) in dense star clusters, which could subsequently evolve into Little Red Dots (LRDs). Our results show that VMS masses can reach $10^3$--$10^4\,M_\odot$, depending on the initial cond
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
- Evolution and surface abundances of red giants experiencing deep mixing#639515
- High-frequency continuous gravitational waves searched in LIGO O3 public data with Einstein@Home#987465
- Boson Stars in Rastall Gravity#202445
- Boson Star Factory: Past, Present, and Future#1061062
- Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes#989187
Record · ID 999803
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