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Table 4.

Position angle of the ionized gas rotating disks and stellar disks.

BGG PAgas PAstellar ΔPA
(°) (°) (°)
Filaments
NGC 193 150.2 ± 0.5 120.2 ± 89.5 30.0
NGC 410 28.9 ± 0.9 185.4 ± 2.3 156.5
NGC 584 92.3 ± 12.7 60.0 ± 0.6 32.3
NGC 677 118.5 ± 6.3
NGC 777 319.3 ± 1.8
NGC 1060 294.9 ± 0.9 16.3 ± 1.4 278.6
NGC 1587 147.4 ± 0.9 231.6 ± 1.3 84.2
NGC 4008 354.6 ± 0.9 168.2 ± 1.4 186.4
NGC 5846 129.3 ± 0.5 306.6 ± 89.5 177.3
NGC 7619 168.0 ± 18.7 217.1 ± 0.9 49.1
Disks
NGC 924 41.6 ± 0.5 52.5 ± 0.9 10.9
NGC 940 198.1 ± 0.5 198.1 ± 0.5 0.0
NGC 978 72.4 ± 0.5 72.4 ± 0.5 0.0
NGC 1453 313.0 ± 0.5 25.3 ± 1.8 287.7
NGC 4169 143.8 ± 0.5 332.9 ± 0.9 189.1
NGC 4261 340.1 ± 5.0 56.1 ± 1.4 284.0
ESO 507-25 163.7 ± 3.2 261.4 ± 3.2 97.7

Notes. The kinetic PA is measured anticlockwise from the north direction to the maximum positive velocity. The errors on the kinetic PA are 3σ errors. ΔPA: difference between the stellar and gas kinematic position angles, ΔPA = |PAstellar − PAgas|.

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