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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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