Table 1: The galaxy sample.
  Type T $B_{\rm T}$ i Bulge typea Environment Runb PAc Exp.d $r_{\rm eff}^{e}$ $\Delta r_{\rm eff}$ $V_{\rm max}^{f}$
NGC 522 Sc 4.1 13.98 90 box   2 123 8200 3.5 0.7 196.1
NGC 585 Sa 1.0 14.06 90 close to box   4,5 86 7200 2.4 0.7 246.6
NGC 678 SBb 3.0 13.31 90 box cluster 1 168 12 000 23.3 1.4 169.0
NGC 891 SAb 3.0 10.83 88 box   1 112 10 500 13.2 0.7 212.0
NGC 973 Sbc 3.2 14.17 90 box   2 138 13 800 3.4 0.4 270.0
NGC 1032 S0-a 0.4 12.74 90 elliptical companions? 1 158 9000 11.4 1.1 283.9
NGC 1184 S0-a 0.0 12.95 90 close to box   2 79 8200 11.3 1.9  
NGC 1351A SBbc 4.5 14.16 80 elliptical cluster 5 132 5400 5.8 0.8 90.7
NGC 1886 Sab 3.9 13.80 90 peanut isolated 3 60 10 800 1.6 0.3 154.6
NGC 3957 SA0 -1.0 13.03 90 close to box cluster 3 173 7200 4.0 0.8  
NGC 5084 S0 -1.8 11.55 90 elliptical cluster 3 80 7200 38.1 11.6 310.3
NGC 6010 S0-a 0.4 12.95 90     1 15 13 800 4.2 0.9 148.8
NGC 6829 Sb 3.0 15.09 90     2 121 12 800 7.1 1.4 211.9
NGC 7183 S0 -0.7 13.14 90 close to box   5 77 7200 2.5 0.5 209.9
NGC 7264 Sb 3.1 14.58 90 elliptical   2 147 13 000 1.2 0.4 248.0
NGC 7332 S0 -2.0 12.56 90 close to box   1 65 15 000 7.5 1.1 121.3
NGC 7396 Sa 1.0 13.85 60 elliptical   2 13 13 000 25.2 1.6 360.7
NGC 7703 S0 -2.0 14.41 90 elliptical cluster 2 57 6400 4.8 2.0 159.5
NGC 7814 SAab 2.0 11.68 67 elliptical   1 45 18 400 33.5 2.0 231.0
IC 1711 Sb 3.0 14.53 90 elliptical   2 133 6200 2.1 0.5 173.4
IC 1970 SAb 3.1 13.36 88 elliptical   4 75 7200 8.1 1.0 118.9
IC 2531 Sb 4.9 12.88 90 peanut cluster 3 75 7200 2.3 0.3 228.1
IC 5176 SABbc 4.4 13.02 90 elliptical companions? 5 151 7200 4.6 0.3 164.2
IC 5264 Sab 2.3 13.58 90 elliptical group 4,5 82 12 600 2.8 0.1 230.6
UGC 10043 Sbc 4.1 15.17 90   cluster 2 61 12 200 1.0 0.3 143.6
UGC 11552 Sab 2.0 15.68 75     5 16 7200 11.7 0.6 243.0
UGC 11587 S0 -1.9 14.52 90     1 76 15 000 5.7 0.7  
ESO 079-003 SBb 3.1 13.91 90 close to box   4,5 134 10 800 5.9 2.0 192.2
ESO 234-053 S0 -1.9 14.32 90     5 81 5400 1.7 0.1  
ESO 311-012 S0-a 0.1 12.38 90 box isolated 3 14 7200 7.4 1.3 95.9
ESO 443-042 Sb 3.1 13.85 90 peanut companions? 3 130 10 800 3.8 0.7 166.3
ESO 512-012 Sbc 3.2 14.42 90 peanut   3 113 5400 1.4 0.3 224.9
a From Lütticke et al. (2000). b Run number in which each galaxy was observed. c Position angle of the long slit. d Total exposure time (in seconds). e Effective radius (in arcseconds) of the bulge, computed as explained in Sect. 4. f Maximum rotational velocity (in km s-1) along the disk major axis, corrected from inclination when necessary. Hubble type T, total apparent magnitude $B_{\rm T}$, galaxy inclination i and $V_{\rm max}$ have been taken from HyperLeda (http://leda.univ-lyon1.fr/).

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