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20 April 2024
 
  » arxiv » 1309.7953

 Article overview


Radiation pressure confinement - II. Application to the broad line region in active galactic nuclei
Alexei Baskin ; Ari Laor ; Jonathan Stern ;
Date 30 Sep 2013
AbstractActive galactic nuclei (AGN) are characterized by broad emission lines. The lines show similar properties from the lowest luminosity (10^39 erg/s) to the highest luminosity (10^47 erg/s) AGN. What produces this similarity over such a vast range of 10^8 in luminosity? Photoionization is inevitably associated with momentum transfer to the photoionized gas. Yet, most of the photoionized gas in the Broad Line Region (BLR) follows Keplerian orbits, which suggests that the BLR originates from gas clouds with a large enough column for gravity to dominate. The photoionized surface layer of these clouds must develop a pressure gradient which balances the incident radiation force. We present solutions for the structure of such a hydrostatic photoionized gas layer in the BLR. The gas is stratified, with a low-density highly-ionized surface layer, set by the ambient pressure, a density rise inwards, and a uniform density cooler inner region, where the gas pressure, 2n_ekT, reaches the incident radiation pressure n_gamma<hnu>, where n_e is the electron density, n_gamma is the photon density, and <hnu> is the mean photon energy. This radiation pressure confinement (RPC) of the photoionized layer leads to a universal ionization parameter U=n_gamma/n_e~0.1 in the inner photoionized layer, independent of distance from the AGN, and of the AGN luminosity. Thus, RPC appears to explain the universality of the BLR properties in AGN. We present predictions for the BLR emission per unit covering factor, as a function of distance from the ionizing source, for a range of ionizing continuum slopes and gas metallicity, which are the only free parameters. The predicted mean strength of most lines, including O VI 1034 and He II 1640 (but excluding H beta), and their peak emissivity radius, are consistent with observations.
Source arXiv, 1309.7953
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