ATLAS. III. Dust around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models

We investigate broad hydrogen line ratios in little red dots (LRDs) using five high-redshift ( z > 2) sources from James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec) medium/high-resolution spectra in the DAWN JWST Archive (DJA) and 15 low-redshift sources ( z = 0.1–0.9) from the literature, all with broad H β detected at >5 σ . After carefully measuring the broad-line fluxes while accounting for absorption features and neighboring emission lines, we find that the broad H α /H β ratios are very high, ranging from 6 to 30, well above the Case B recombination value. Using plane-parallel C loudy 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 H α /H β –Pa β /Pa γ 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 H α /H β 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 H α /H β > 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 active galactic nuclei, reconciling the weak hot-dust emission.