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Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the Black Hole Mass-Velocity Dispersion Relationship for Active Galactic Nuclei

机译:活跃银河核中的超大质量黑洞。二。活跃银河核黑洞质量-速度色散关系的校准

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We calibrate reverberation-based black hole (BH) masses in active galactic nuclei (AGNs) by using the correlation between BH mass, MBH, and bulge/spheroid stellar velocity dispersion, σ*. We use new measurements of σ* for six AGNs and published velocity dispersions for 10 others, in conjunction with improved reverberation-mapping results, to determine the scaling factor required to bring reverberation-based BH masses into agreement with the quiescent galaxy MBH-σ* relationship. The scatter in the AGN BH masses is found to be less than a factor of 3. The current observational uncertainties preclude the use of the scaling factor to discriminate between broad-line region models.
机译:我们通过利用BH质量MBH和凸出/椭球体恒星速度色散σ*之间的相关性来校准活跃银河原子核(AGN)中基于混响的黑洞(BH)质量。我们使用了六个AGN的σ*的新测量值以及另外十个AGN的已公布速度色散,并结合了改进的混响映射结果,来确定使基于混响的BH质量与静态星系MBH-σ*一致所需的比例因子。关系。发现AGN BH块中的散射小于3倍。当前的观测不确定性排除了使用缩放因子来区分宽线区域模型的可能性。

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