Astronomy & Astrophysics

Table 1: Basic properties of 3C 48.
Table 2: Initial parameters of the two identical galaxies in the system of units suitable for 3C 48. Each galaxy consists of a spherical non-rotating bulge, a rotating exponential disk, and an isothermal halo (Hernquist 1993).
Table 3: Measured proportions of the 3C 48 host, as taken from the contour plot in Fig. 1 of Canalizo & Stockton (2000), compared to the proportions of the nearest look-alike.