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Table 2.

Rotation amplitude VGCS and velocity dispersion σGCS for the GC systems of the F3D galaxies.

Galaxy σe Nred Nblue VGCS σGCS Vred, GCS σred, GCS Vblue, GCS σblueGCS
(km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
FCC083 103 20 37 82.8 97.1 110.3 64.0 61.6 113.4
FCC143 62 0 20 18.2 59.7
FCC147 131 22 30 43.4 131.1 40.3 152.6 61.6 118.6
FCC153 55 1 13 48.2 68.0 44.3 69.9
FCC161 96 22 48 22.1 90.9 26.7 67.0 23.5 101.7
FCC167 143 38 21 117.4 172.4 118.2 198.2 115.6 123.5
FCC170 113 4 18 33.3 122.9 25.6 127.5
FCC176 43 1 10 29.5 51.0 33.4 53.8
FCC177 42 3 16 40.5 51.4 49.5 49.0
FCC184 143 40 9 57.9 68.3 57.9
FCC190 75 5 27 42.7 101.6 53.3 109.1
FCC193 95 7 9 134.6 128.5
FCC213 68 41 51.8 228.8 30.3 192.5 102.1 282.0
FCC219 154 17 7 119.6 175.5 118.5 197.9
FCC249 104 5 24 24.7 96.0 26.4 100.4
FCC255 38 1 18 22.2 36.0 22.8 37.1
FCC276 123 18 35 29.2 140.5 34.3 123.4 34.3 153.2
FCC310 48 2 11 30.8 59.5 26.9 67.1

Notes. (1) Galaxy name. (2) Average LOS velocity dispersion within 1 Reff from Iodice et al. (2019a). (3) and (4) Number of red and blue GCs in the F3D sample. (6)−(10) Rotation amplitude and velocity dispersion. If ten or more GCs are available in the red and blue populations, we determined VGCS and σGCS for these separately.

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