Fig. 6
Luminosity λ and accretion rate ṁ for large, non-advective PDs with constant angular momentum. The luminosity integrated over whole torus is indicated with a thick line, while the thin line corresponds to the funnel luminosity (i.e., integrated over R < Rmax). The dash-dotted lines correspond to the asymptotic formulae for very thick tori, Eqs. (46), (47).
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