Is. Yi et al., ON THE ORIGIN OF OBSCURING TORI IN THE GALACTIC NUCLEUS AND ACTIVE GALACTIC NUCLEI, The Astrophysical journal, 432(1), 1994, pp. 120000031-120000034
Differences between Seyfert 1 and Seyfert 2 galaxies can be explained
by the existence of obscuring tori at distances a few parsecs from cen
tral black holes. In the Galaxy there exists a similar thick disk stru
cture, the circumnuclear disk, at a distance approximately 1.7 pc from
the Galactic center. We examine the possibility that both structures
are the result of turbulence-supported viscous evolution and accumulat
ion of accreted material in soft gravitational potentials of galactic
nuclei. The accumulation occurs in a region where the gravitational po
tential provides reduced differential rotation compared with different
ial rotation in the neighboring regions. The existence of these struct
ures requires that the ratio of the smooth background mass within appr
oximately a few parsecs to the central black hole mass be of order 1.
We also discuss how strong magnetic fields prevent such tori formation
and suggest evolutionary possibilities consistent with our results.