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Table 3:

Kinematic properties of the sample

(1) 		(2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
HCG Galaxy PA $_{\rm {kin}}$ PA $_{\rm {morph}}$ PA $_{\rm {morph}}$ $i_{\rm {kin}}$ $i_{\rm {morph}}$ $i_{\rm {morph}}$ $V_{\rm {sys HICK}}$ $V_{\rm {sys FP}}$ vvir $\delta$ $c_{\rm {kin-morph}}$
    deg deg deg deg deg deg km s-1 km s-1 km s-1 arcsec
2 a 42 $\pm$ 4 3 8 $\pm$ 13 68 $\pm$ 13 61 $\pm$ 2 65 4326 4347 4375 42.2
  b 5 $\pm$ 3 28 3 $\pm$ 90 49 $\pm$ 12 30 $\pm$ 21 43 4366 4357 4365 1.3
  c 168 $\pm$ 4 132 158 $\pm$ 18 ... 57 $\pm$ 3 64 4235 4266 4284 2.4
7 a 179 $\pm$ 2 153 165 $\pm$ 13 67 $\pm$ 3 61 $\pm$ 2 76 4210 4198 4178 0.6
  d 85 $\pm$ 3 58 35 $\pm$ 34 31 $\pm$ 12 43 $\pm$ 7 44 4116 4104 4081 12.3
22 c 101 $\pm$ 2 70 179 $\pm$ 90 ... 25 $\pm$ 14 90 2728 2572 2444 6.8
37 d 68 $\pm$ 4 58 108 $\pm$ 90 60 $\pm$ 15 38 $\pm$ 29 36 6207 6308 6236 0.8
40 c 120 $\pm$ 2 125 134 $\pm$ 8 74 $\pm$ 4 75 $\pm$ 2 90 6890 6888 6341 1.6
  e 8 $\pm$ 10 72 57 $\pm$ 21 ... 70 $\pm$ 6 80 6625 ... 6383 0.0
47 a 42 $\pm$ 3 42 14 $\pm$ 25 24 $\pm$ 11 47 $\pm$ 5 67 9581 9507 9622 ...
  d 15 $\pm$ 1 165 174 $\pm$ 54 16 $\pm$ 4 39 $\pm$ 12 32 9471 9325 9533 ...
49 a 42 $\pm$ 8 57 49 $\pm$ 90 18 $\pm$ 10 22 $\pm$ 23 43 9939 9812 10196 9.1
  b 91 $\pm$ 3 72 85 $\pm$ 31 51 $\pm$ 7 49 $\pm$ 7 59 9930 9787 10190 4.5
  c 175 $\pm$ 4 98 100 $\pm$ 90 11 $\pm$ 6 39 $\pm$ 31 45 9926 9784 10185 23.7
56 a 174 $\pm$ 1 172 173 $\pm$ 7 75 $\pm$ 3 75 $\pm$ 1 90 8245 8374 8455 1.6
68 c 31 $\pm$ 1 119 34 $\pm$ 25 30 $\pm$ 4 36 $\pm$ 4 54 2313 2515 2550 1.0
93 b 173 $\pm$ 4 156 39 $\pm$ 8 79 $\pm$ 6 70 $\pm$ 1 68 4672 4625 4776 1.3
  NGC 92 146 $\pm$ 2 149 149 $\pm$ 12 48 $\pm$ 6 63/62 $\pm$ 2 70 3219 3412 3132 0.7

Notes. Column (1): group number. Column (2): Galaxy member of the group. Column (3): PA deduced from our velocity field. Column (4): PA taken from Mendes de Oliveira (1992) for HCG. This was determinated for semimajor axis lengths of 2 h-1 kpc for all Hickson group galaxies with z $\leq$ 0.05. Column (5): optical PA taken from HyperLeda. PA is the position angle of the major axis of the isophote 25 mag arcsec-2 in the B-band. Column (6): inclination deduced from the analysis of our velocity field. Column (7): morphological inclination deduced from the axis ratio of the isophote 25 mag arcsec-2 in the B-band for galaxies ( $\rm {cos}\it {(b/a)}=\it {i}$). For NGC 92 given values correspond to HyperLeda/NED. Column (8): morphological inclination taken from HyperLeda. Column (9): systemic velocity taken from Hickson (1993). Column (10): systemic velocity deduced from our velocity field analysis. Column (11): radial velocity corrected by the Virgo infall from HyperLeda. Column (12): difference in arcseconds between the morphologial and kinematic centers.


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