- 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
flux in 10-15 erg s-1 cm-2 found by Conselice et al. (2001) in the region identified in the Fig. 3.