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Ma, Z · 2026 · arXiv (Cornell University) · DOI 10.48550/arxiv.2601.15962 · arXiv 2601.15962

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astro-ph.GA 2

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

The quasi-star model for Little Red Dots: potential and challenges

astro-ph.GA · 2026-06-04 · unverdicted · novelty 5.0

Quasi-star models using Cloudy radiative transfer reproduce the UV-NIR continuum shape, Balmer break, and hydrogen line luminosities in some LRDs when combined with host galaxy emission, but fail to account for broad helium lines and hot dust without added components.

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Showing 2 of 2 citing papers.

  • The quasi-star model for Little Red Dots: potential and challenges astro-ph.GA · 2026-06-04 · unverdicted · none · ref 53 · internal anchor

    Quasi-star models using Cloudy radiative transfer reproduce the UV-NIR continuum shape, Balmer break, and hydrogen line luminosities in some LRDs when combined with host galaxy emission, but fail to account for broad helium lines and hot dust without added components.

  • Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys astro-ph.GA · 2026-06-29 · unverdicted · none · ref 46 · internal anchor

    SKAO continuum surveys will detect radio emission from JWST AGN and LRDs and distinguish between Compton-thick absorption, intrinsically weak accretion, and dense gas cocoon scenarios.