Table 3.
Properties of the kinematically disturbed H I gas.
| Source (a) | Component (b) |
 (c) |
NH I(d) | d(e) | nH I(f) | mH I(g) | v(h) | r⋆(i) | ṀH I(j) |
|---|---|---|---|---|---|---|---|---|---|
| [1019 cm−2 K−1] | [1019 cm−2] | [pc] | [cm−3] | [104 M⊙] | [km s−1] | [pc] | [M⊙ yr−1] | ||
| 4C 12.50 | Outflow | 4.6 | 460 | 50 × 12 | 150−300 | 1.6 | 1000 | – | 16−29 |
| 4C 52.37 | Outflow | 2.0 | 2000 | ≲38 | 170 | 18 | 450 | ≲38 | 4.3 |
| Systemic | 1.0 | 1000 | 95 × ≲38 | 85 | 23 | – | – | – | |
| 3C 236 | Outflow (Core) | 0.78 | 780 | ≲36 | 120 | 2.8 | 640 | ≲40 | 0.5 |
| 3C 293 | Outflow (Core) | 0.4 | 400 | ≲24 | 54 | 1.5 | 300 | ≲24 | 0.36 |
| Systemic (Core) | 2.0 | 2000 | 33 × 33 | 196 | 1.4 | – | – | – |
Notes.
Values for 4C 12.50 from Morganti et al. (2013), for 3C 236 from Schulz et al. (2018), and for 4C 52.37 and 3C 293 from this paper. For 4C 12.50 and 3C 236, we focus on the kinematically disturbed H I gas.
Mean H I column density. Tspin = 1000 K is assumed except for 4C 12.50 for which Morganti et al. (2013) assumed Tspin = 100 K.
Projected size of the components. For the outflow, a spherical geometry is assumed with an upper limit of the diameter based on the synthesized beam. For S1, an ellipsoidal geometry is assumed, with the major and minor axis given.
Mass outflow rate following Heckman (2002) for the chosen Tspin values.
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