Table 1: Observed and derived dust properties of our target galaxies.
Target D Total observed Flux $T_{\rm dust,disk}$ $M_{\rm dust,disk}$ $T_{\rm dust,center}$ $M_{\rm dust,center}$ $M_{\rm gas,total}^{a}$
  [Mpc] [Jy] [K] [106 $M_{\odot}$] [K] [106 $M_{\odot}$] [109 $M_{\odot}$]
NGC 253 2.5 $17.6\pm1.8$ 17/28 11.7 35/55 2.0 2.1
NGC 4945 3.8 $15.8\pm1.6$ 17/28 19.8 20/40 5.7 4.2
NGC 5128 3.5 $18.0\pm1.7^{b}$ 20/30 8.0 14/30 10.8 2.8
a Assuming a gas-to-dust mass ratio of 150;
b non thermal contribution: 6.4 Jy (nucleus), 3.3 Jy (radio lobes).

Source LaTeX | All tables | In the text