All Tables

Table 1: Parameters for NGC 1275 (at the distance of 77 Mpc adopted for NGC 1275, 1 arcsec = 0.37 kpc).
Table 2: Intensity of the CO(2-1) emission lines in the Shields and Filippenko star cluster region. Two Gaussians have been fitted. Around half of the total area is found in a broad line (300 km s^-1) and the other half is found in a narrower (130 km s^-1) component. The stronger emission could be associated with the star cluster and the smaller one with the underlying filament.
Table 3: Parameters of the brigthest CO(2-1) emission lines plotted in Fig. 3. The first and second columns give the region number as used in the related plots and the corresponding position offset in arcsec relative to the cD coordinates. The 3rd, 4th, 5th, 6th, 7th columns list the line parameters of fitted Gaussian profiles. The center of the lines is taken by comparison with the cD rest frame (z=0.01756). In Col. 8, we computed the cold molecular mass for each region, as explain in the text. Finally, the last column list the H $\alpha$ flux in 10^-15 erg s^-1 cm^-2 found by Conselice et al. (2001) in the region identified in the Fig. 3.