2024ApJ...961...82Z

Strong evidence is reported to support unobscured broad-line regions (BLRs) in Type-1.9 active galactic nucleus (AGN) SDSS J1241+2602 with reliable broad Hα but no broad Hβ. Commonly, the disappearance of broad Hβ can be explained by the AGN unified model, in which heavily obscured BLRs are expected in Type-1.9 AGNs. Here, based on properties of two kinds of BH masses, the virial BH mass and the BH mass obtained through the M_BH-σ relation, an independent method is proposed to test whether there are unobscured central BLRs in a Type-1.9 AGN. By the reliable measurement of stellar velocity dispersion of about 110 ± 12 km s ^–1 through the host galaxy absorption features in SDSS J1241+2602, the BH mass obtained through the M_BH-σ relation is consistent with the virial BH mass (3.43 ± 1.25) × 10⁷M_⊙ determined through properties of the observed broad Hα without considering the effects of obscurations in SDSS J1241+2602. Meanwhile, if considering heavily obscured BLRs in SDSS J1241+2602, the reddening-corrected virial BH mass is tens of times larger than the value expected from M_BH-σ, leading SDSS J1241+2602 to be an outlier in the M_BH-σ space with a confidence level higher than 5σ. Therefore, unobscured BLRs are preferred in the Type-1.9 AGN SDSS J1241+2602. The results indicate that it is necessary to check whether unobscured central BLRs are common in Type-1.9 AGNs when testing the unified model of AGNs through properties of Type-1.9 AGNs.