{ "id": "1606.03303", "version": "v1", "published": "2016-06-10T13:01:28.000Z", "updated": "2016-06-10T13:01:28.000Z", "title": "Physical properties and the variability mechanism of the He I outflow in NGC 4151", "authors": [ "Conor Wildy", "Hermine Landt", "Michael R. Goad", "Martin J. Ward", "James S. Collinson" ], "comment": "Accepted for publication in MNRAS. 17 pages, 15 figures", "categories": [ "astro-ph.GA" ], "abstract": "We report on variable helium absorption lines in NGC 4151 observed across six epochs of quasi-simultaneous near-infrared and optical data. These observations cover the transitions from the metastable 2^3S state at 3889 A and 10830 A, and from the 2^1S state at 20587 A. This is the first AGN absorption line variability study to include measurements of the 20587 A line. The physical properties of the absorber recorded at the fifth observational epoch are relatively well constrained by the presence of absorption in both the optical and near-infrared components, with the 10830 A line likely saturated. The observations suggest variations in this absorber's strength are best explained by ionization changes in response to a variable incident continuum. Photoionization simulations constrain the total hydrogen number density of the epoch 5 absorber to 7.1