ATLAS. III. Dust Around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models
Abstract
We investigate broad hydrogen line ratios in little red dots (LRDs) using five high-redshift (z>2) sources from JWST/NIRSpec medium/high-resolution spectra in the DAWN JWST Archive and fifteen low-redshift sources (z=0.1--$0.9$) from the literature, all with broad Hβ detected at >5σ. After carefully measuring the broad-line fluxes while accounting for absorption features and neighboring emission lines, we find that the broad Hα/Hβ ratios are very high, ranging from 6 to 30, well above the Case B recombination value. Using plane-parallel \textsc{Cloudy} photoionization models with the total line emission from both sides of the slab, we investigate the physical origin of the broad hydrogen line ratios beyond Case B, jointly modeling the Balmer and Paschen line ratios for the subset of one high-z and two low-z LRDs with detected broad Paschen lines. We find that one low-z LRD is reproduced by a high gas number density (log (nH/cm−3)∼10--11) on the broad-line Hα/Hβ--Paβ/Paγ plane, whereas the remaining two LRDs additionally require substantial dust extinction of E(B−V)≳0.2, even after accounting for non-Case B effects. Since the narrow Hα/Hβ ratios do not indicate such large dust extinction, these results demonstrate that the obscuring dust is spatially associated with the broad-line region. Even without Paschen-line measurements, two and eight LRDs in the high- and low-redshift samples, respectively, exhibit Hα/Hβ>13, which cannot be reproduced by the non-Case B models, suggesting that dust obscuration might be common among LRDs, occurring in at least about half of the population. Such dust may represent a lower-column-density counterpart of the dusty torus in AGNs, reconciling the weak hot-dust emission.
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BibTeX
@misc{kiyota2026atlas,
title = {{ATLAS. III. Dust Around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models}},
author = {Tomokazu Kiyota and Masami Ouchi and Hiroto Yanagisawa and Makoto Ando and Yuichi Harikane and Yuta Kageura and Minami Nakane and Yurina Nakazato and Yoshiaki Ono and Yui Takeda},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2608.10832},
eprint = {2608.10832},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2608.10832},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - ATLAS. III. Dust Around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models
AU - Tomokazu Kiyota
AU - Masami Ouchi
AU - Hiroto Yanagisawa
AU - Makoto Ando
AU - Yuichi Harikane
AU - Yuta Kageura
AU - Minami Nakane
AU - Yurina Nakazato
AU - Yoshiaki Ono
AU - Yui Takeda
PY - 2026
DA - 2026/10/15
PB - arXiv
DO - 10.48550/arxiv.2608.10832
UR - https://arxiv.org/abs/2608.10832
AB - We investigate broad hydrogen line ratios in little red dots (LRDs) using five high-redshift (z>2) sources from JWST/NIRSpec medium/high-resolution spectra in the DAWN JWST Archive and fifteen low-redshift sources (z=0.1--$0.9$) from the literature, all with broad Hβ detected at >5σ. After carefully measuring the broad-line fluxes while accounting for absorption features and neighboring emission lines, we find that the broad Hα/Hβ ratios are very high, ranging from 6 to 30, well above the Case B recombination value. Using plane-parallel \textsc{Cloudy} photoionization models with the total line emission from both sides of the slab, we investigate the physical origin of the broad hydrogen line ratios beyond Case B, jointly modeling the Balmer and Paschen line ratios for the subset of one high-z and two low-z LRDs with detected broad Paschen lines. We find that one low-z LRD is reproduced by a high gas number density (log (n_H/cm^−3)∼10--11) on the broad-line Hα/Hβ--Paβ/Paγ plane, whereas the remaining two LRDs additionally require substantial dust extinction of E(B−V)≳0.2, even after accounting for non-Case B effects. Since the narrow Hα/Hβ ratios do not indicate such large dust extinction, these results demonstrate that the obscuring dust is spatially associated with the broad-line region. Even without Paschen-line measurements, two and eight LRDs in the high- and low-redshift samples, respectively, exhibit Hα/Hβ>13, which cannot be reproduced by the non-Case B models, suggesting that dust obscuration might be common among LRDs, occurring in at least about half of the population. Such dust may represent a lower-column-density counterpart of the dusty torus in AGNs, reconciling the weak hot-dust emission.
ER -