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Table A.1.

Model parameters and their meaning.

large scale disk CND NGC 1068
vrot(20 pc) 100 km s−1 100 km s−1 rotation velocity
(Guesten et al. 1987; Hicks et al. 2009)
vA, 0 1.0 km s−1 1.5 km s−1 Alfven velocity (Vollmer & Davies 2013)
Mdyn(20 pc) 4.4 × 107 M 4.4 × 107 M total enclosed (dynamical) mass
(Genzel et al. 2010; Hicks et al. 2009)
Mgas 4.5 × 104 M 3.6 × 105 M total gas mass (this work)
vturb 20 km s−1 50 km s−1 gas turbulent velocity dispersion
(Guesten et al. 1987; Hicks et al. 2009)
Q 300 30 disk Toomre parameter (Eq. A.1)
3.8 Myr−1 2 × 10−3 Myr−1 disk mass accretion rate (this work)
η 0.1 0.1 dissipated energy fraction per cloud-cloud
collision (Sect. 2.1)
α 3.7 × 1013 cm3s−1g−1 3.7 × 1013 cm3s−1g−1 gas particle collision coefficient
(Draine 1983)
γ ion-neutral coupling
(Williams et al. 1998, McKee et al. 2010)
ζCR 2 × 10−15 s−1 2 × 10−13 s−1 cosmic ray ionization rate
(Yusef-Zadeh et al. 2013, this work)
LX 0 5 × 1043 erg s−1 X-ray luminosity (Bauer et al. 2015)
MBH 4 ×106 M 1 ×107 M black hole mass (Genzel et al. 2010
Greenhill et al. 1996)
R galactic radius
Ω angular velocity
ρ disk midplane density
Σ disk surface density
H disk height
ldriv turbulent driving lengthscale
ΦV cloud volume filling factor (Eq. A.5)
ΦA cloud area filling factor (Eq. A.8)
xi ionization fraction (Eq. A.4)
ζX X-ray ionization rate (Eq. 10)
Γg gas heating rate (Eq. 5)
Γturb turbulent heating rate (Eq. 6)
ΓCR cosmic ray heating rate (Eq. 8)
ΓX X-ray heating rate (Eq. 7)
HX X-ray energy deposition rate per
particle (Eq. 9)

small scale clouds

rsh compression rate of the C-shock (Eq. A.2)
Mcl cloud mass
rcl cloud radius (Eq. A.3)
lcl cloud size
ρcl cloud density
Ncl cloud surface density
cs local sound speed
cloud free fall time
Tg gas temperature
B magnetic field

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