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Table 3:

Properties of the central emission peaks.
UGC NGC Classn. Dist. Peak Res FWHM
      Mpc     kpc
3685 - SB(rs)b 26 Y U <0.17
4273 2543 SB(s)b 35 Y R 0.65
4484 2608 SB(s)b 32 Y R 0.34
4574 2633 SB(s)b 31 Y R 0.62
47051 2710 SB(rs)b 36 Y R+ 1.10
4708 2712 SB(r)b: 29 Y R+ 1.20
6077 3485 SB(r)b: 27 Y R 0.29
61232 3507 SB(s)b 21 Y R? -
65953 3769 SB(r)b: 12 Y R+ 0.32
7002 4037 SB(rs)b: 18 Y R? 0.24
75234 4394 (R)SB(r)b: 18 Y R+ 0.46
77535 4548 SB(rs)b 18 Y R+ 0.45
96496 5832 SB(rs)b? 8 N - -
126997 7714 SB(s)b:p 31 Y R? 0.32
1 Emission elongated along bar axis. 2 LINER; foreground star contamination, so not in mean profiles. 3 Interacting with NGC 3769A, type Sm. 4 LINER; Smooth extended emission, possible ENER. 5 M91; LINER/Seyfert; possible ENER. 6 Classified as SBc in UGC. 7 H II/LINER; tidally distorted.
For each galaxy, we list the UGC and NGC catalogue numbers, the full galaxy classifications from de Vaucouleurs et al. (1991), the distance in Mpc from Paper I, whether or not the galaxy exhibits a central peak in H$\alpha $ emission, the resolution of the peak as explained in Sect. 4.2, and the FWHM of the emission, in kpc. All LINER/Seyfert classifications in the footnotes are taken from the NASA/IPAC Extragalactic Database (NED).

Source LaTeX | All tables | In the text

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