All Tables

Table 1: High spatial resolution observations of the nulear emission of NGC 1068 from radio to infrared frequencies.
Table 2: Parameters of the synchrotron models A, B, and C for the nuclear source S1 of NGC 1068: the linear scale s is the half thickness in model A & B and the radius of the emission spheres in model C. For the mean Lorentz factor $\left <\gamma \right >$ of the electron distributions (width $\Delta \gamma /\left <\gamma \right > = 2$ ) there are only lower limits derived form the assumed upper cut-off frequency $\nu _{\rm c} = 3\times 10^{14}$ Hz of the synchrontron spectrum. The values for $B_{\rm Min}$ is the minimum energy B-field for the claimed size of s=5.6 mas in model A and upper limits for B and C. The electron density in the last column corresponds to $B_{\rm Min}$ .
Table 3: Parameters for the free-free emission model described in the text.