arXiv (OAI Expanded)
open access
Little Red Dots as Supermassive Counterparts of SS 433: A Hyper-Eddington Accretion Framework
High-redshift little red dots (LRDs) are compact sources characterized by V-shaped spectral energy distributions (SEDs), broad emission lines, and often prominent Balmer breaks. Their high number density and apparently large black hole masses suggest that they are essential to the early evolution of
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
- Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses#985073
- A Population of Little Red Dot-like Quasars in SDSS#997508
- Do little red dots really form a distinct class of astronomical objects?#984144
- A direct black-hole mass measurement in a little red dot at high redshift#1066036
- Free-Free Radio Emission from Little Red Dots as a Probe of Ionized Gas#1034887
Record · ID 1084259
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