Table 4.
Position angles (PAs).
| Galaxy | Maser disk | 5 GHz jet direction | Jet offset | 33 GHz continuum | Galaxy scale | Ref. | |
|---|---|---|---|---|---|---|---|
| (°) | (°) | (°) | (°) | (°) | |||
| Mrk 0001 | 6.4 ± 10 | 113 ± 5 | 17 ± 11 | 120 ± 2 | 77.5 | 1 | |
| Mrk 1210 | 62.58 ± 0.45 | 127 ± 22 | 26 ± 22 | 179 ± 83 | 160.0 | 2 | |
| Mrk 1419 | 49 ± 0.7 | 159 ± 2 | 20 ± 1 | 117 ± 84 | 40.2 | 3 | |
| NGC 2273 | 153 ± 4.6 | 95 ± 1 | 32 ± 5 | 83 ± 3 | 63.3 | 3 | |
| UGC 3193 | – | 175 ± 0.2 | – | 167 ± 4 | 177.4 | – |
Notes. Column 1: name of galaxy. The sources in bold hold clean maser disks (see Sect. 2). Column 2: maser disk PAs and their uncertainties. Column 3: jet propagation direction, obtained from a linear fit on the position of the flux maxima in multicomponent sources (see Sect 5.1). If there is only one component, the 5 GHz continuum PA of this component represents the jet propagation direction. Column 4: PA difference between the disk rotation axis (the normal vector to the disk) and jet propagation direction and the uncertainties. Column 5: 33 GHz larger scale PAs from Kamali et al. (2017). Column 6: large-scale galactic disk PA from HyperLeda. Column 7: references for maser disk PA. (1) Kuo et al. (in prep.); (2) Zhao et al. (2018); (3) Kuo et al. (2011).
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