arXiv (All)
open access
The role of major mergers in triggering super-Eddington accretion
JWST observations have opened a new era in the exploration of the high-redshift Universe, revealing black holes (BHs) with masses of several million solar masses already at $z>8$, challenging our understanding of their growth mechanisms. In this context, super-Eddington (SE) accretion has emerged as
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
- Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe#1122902
- Hierarchical Black Hole Mergers at High Redshift: Predictions for LISA and LGWA from SEEDZ#1216558
- Super-Eddington Accretion and Early-Stage Feedback in Ton S180#927613
- Semi-Analytic Solutions For Warped, Super-Eddington Accretion Disks with Outflows#1064561
- The Quasar Main Sequence of Super-Eddington NLSy1 Galaxies#652349
Record · ID 1413693
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