Line width distributions as evidence for axisymmetry in the broad line regions of active galaxies

Details Line width distributions as evidence for axisymmetry in the broad line regions of active galaxies Line width distributions as evidence for axisymmetry in the broad line regions of active galaxies

1998-04-20

arxiv.org/abs/astro-ph/9804192v1

Astronomy and Astrophysics

Astrophysics

8 pages including 4 figures. Accepted for publication in MNRAS Letters

Scientific paper

10.1046/j.1365-8711.1998.01672.x

The nuclei of a wide class of active galaxies emit broad emission lines with widths at half maximum (FWHM) in the range $10^{3}-10^{4}$ km s$^{-1}$. This spread of widths is not solely a consequence of the range of the luminosities of these sources since a plot of width versus luminosity shows a large scatter. We propose that the broad line emission region (BLR) is axially symmetric and that this scatter in line width arises from an additional dependence on the angle of the line of sight to the axis of the emission region. Such a relation is natural in unified models of active nuclei which link a variety of observed properties to viewing angle. Adopting a simple form for the line width as a function of luminosity and angle, and convolving this with the observed luminosity function, allows us to predict a line width distribution consistent with the available data. Furthermore, we use the relation between the equivalent width of a line and the luminosity in the continuum (the `Baldwin Effect') to predict an observed correlation between line width and equivalent width. The scatter on this correlation is again provided by angular dependence. The results have applications as diagnostics of models of the broad line emission region and in cosmology.

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