arXiv (All)
open access
JWST's Little Red Dots as collapsed Supermassive Dark Stars
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-phenomenology
The nature of the ``Little Red Dots'' (LRDs) is one of the most profound mysteries posed by the JWST data. One promising class of models that can reproduce the observed LRDs spectra and morphology are quasi-stars: massive envelopes surrounding accreting black holes formed via the collapse of superma
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 are Direct-Collapse Black Hole-Forming Galaxies#1000022
- What is the nature of GW230529? An exploration of the gravitational lensing hypothesis#1049588
- Testing the wormhole echo hypothesis for GW231123#1155109
- Long-term X-ray spectral analysis of Cygnus X-1 using AstroSat#1000045
- Direct imaging of sub-parsec binary SMBHs in the central galaxy of the NGC 5044 group#1037116
Record · ID 986267
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