arXiv (OAI Expanded)
open access
The quasi-star model for Little Red Dots: potential and challenges
(Abridged) Little Red Dots (LRDs) are a class of sources discovered by JWST observationally defined by a "V-shaped" rest-frame UV-Optical SED, a compact or unresolved morphology, and for having, frequently, broad hydrogen emission lines. Among various models, those involving a quasi-star interpret L
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
- Exploring the observed properties of JWST Little Red Dots with cosmological simulations and dust radiative transfer#1129514
- Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses#985073
- An Updated Infrared Solar Spectrum from ACE-FTS and a CH Rovibrational Line List#453053
- The Post-Outburst Spectrum of L1415-IRS#1110689
- Reigniting the FUSE II: O VI Emission in Massive Elliptical Galaxies#1071164
Record · ID 1069814
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