All Tables

Table 1: Comparison between our photometry JB (Johansson & Bergvall 1990) and other published data. $\Delta V$ , $\Delta (B-V)$ and $\Delta (U-B)$ are the differences between our data and the other published data.
Table 2: Heliocentric velocities and formal mean errors of the galaxies in the IG sample. n is the number of absorption (a) and emission (e) lines used in the determination of the velocities.
Table 3: Heliocentric velocities and formal mean errors of the galaxies in the IG sample, continued.
Table 4: Heliocentric velocities and mean errors of the galaxies in the NIG sample.
Table 5: Fluxes of the most prominent emission lines of the optical centres of the interacting and merging galaxies. The size of the aperture was $1.5\hbox {$^{\prime \prime }$ }\times 3\hbox {$^{\prime \prime }$ }$ . The unit is 10^-19 W m^-2. Positive numbers are emission lines and negative are absorption lines.
Table 6: Fluxes of the most prominent emission lines of the galaxies in the comparison sample. The unit is 10^-19 W m^-2. Positive numbers are emission lines and negative are absorption lines. Only galaxies with detected emission lines are included.