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- W2546846300 abstract "We study AGN emission line profiles combining an improved version of the accretion disc-wind model of Murray & Chiang with the magnetohydrodynamic (MHD) model of Emmering et al. Here, we extend our previous work to consider central objects with different masses and/or luminosities. We have compared the dispersions in our model C iv line-width distributions to observational upper limit on that dispersion, considering both smooth and clumpy torus models. Following Fine et al., we transform that scatter in the profile line-widths into a constraint on the torus geometry and show how the half-opening angle of the obscuring structure depends on the mass of the central object and the accretion rate. We find that the results depend only mildly on the dimensionless angular momentum, one of the two integrals of motion that characterize the dynamics of the self-similar ideal MHD outflows." @default.
- W2546846300 created "2016-11-11" @default.
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- W2546846300 date "2016-10-12" @default.
- W2546846300 modified "2023-10-17" @default.
- W2546846300 title "Magnetohydrodynamic disc winds and line width distributions – II" @default.
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- W2546846300 doi "https://doi.org/10.1093/mnras/stw2626" @default.
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