Table 4.
Sizes, masses, and orientations of the extended components of continuum emission.
| Name | Size (a) | log (b) |
log (c) |
 (d) |
PAGauss(e) | PAout(f) | Ωout(f) | Δ(g) | Geometry (h) |
|---|---|---|---|---|---|---|---|---|---|
| pc | M⊙ | M⊙ | mol. cm−2 | ° | ° | ° | ° | — | |
| (MSR, HSR) | (MSR, HSR) | (MSR, HSR) | (MSR, HSR) | (MSR, HSR) | – | – | (MSR, HSR) | – | |
| NGC 6300 | (64, 53) | (6.5, 6.6) | (6.8, 6.7) | (23.4, 23.4) | (85, 85) | 18 | 95 | (67, 67) | Torus |
| NGC 5643 | (43, 41) | (6.3, 6.5) | (6.7, 6.7) | (23.6, 23.6) | (4, 5) | 83 | 105 | (79, 78) | Torus |
| NGC 7314 | (60, 50) | (5.9, 5.8) | (5.8, 5.7) | (22.1, 22.1) | (21, 30) | −70 | 95 | (89, 80) | Torus |
| NGC 4388 | (32, 29) | (6.0, 6.0) | (5.5, 5.4) | (22.3, 22.4) | (−43, −7) | 15 | 100 | (58, 22) | Mixed/polar |
| NGC 4941 | (78, 74) | (5.9, 6.0) | (5.9, 5.7) | (21.9, 21.9) | (−27, −29) | −59 | – | (32, 30) | Mixed/polar |
| NGC 7213 | (40, 34) | (7.5, 7.4) | (4.8, 4.5) | (< 22.0, < 22.3) | (71, 44) | -19 | – | (90, 63) | Torus |
| NGC 7582 | (91, 82) | (6.4, 6.6) | (6.6, 6.5) | (22.6, 22.5) | (−18, −20) | 58 | 95 | (76, 78) | Torus |
| NGC 6814 | (33, 39) | (5.7, 5.8) | (4.9, 4.9) | (< 21.8, < 22.3) | (90, 61) | 33 | 115 | (57, 28) | Mixed/polar |
| NGC 5506 | (129, 91) | (6.7, 6.9) | (7.0, 6.7) | (22.6, 22.7) | (87, 88) | 17 | 85 | (70, 71) | Torus |
| NGC 7465 | (67, 56) | (6.2, 6.3) | (6.3, 6.2) | (22.6, 22.7) | (4, 4) | −72 | 95 | (76, 76) | Torus |
| NGC 1068 | 26 | 5.0 | 5.5 | 23.6 | −55 | 30 | 80 | 85 | Torus |
| NGC 1365 | 28 | 6.2 | 5.4 | 22.3 | 50 | −45 | 110 | 85 | Torus |
| NGC 3227 | 41 | 6.3 | 6.2 | 22.7 | −14 | 35 | 90 | 49 | Mixed |
Notes.
Deconvolved diameters of the extended components derived from the MSR and HSR continuum datasets of the GATOS core sample (listed first); we also include fits to the data of NGC 1068 (García-Burillo et al. 2016), NGC 1365 (Combes et al. 2019), and NGC 3227 (Alonso-Herrero et al. 2019).
Molecular gas masses derived from the continuum emission of the extended components (see details in Sect. 4).
Position angle of the elliptical Gaussian fits to the extended components (see details in Sect. 4).
Position angle (PAout) and opening angle (Ωout) of the ionized outflows (see references in Appendix A and Sect. 2).
Projected relative orientation angle between the extended component and the outflow axis, defined as Δ≡ min[|PAGauss − PAout|, 180° −|PAGauss − PAout|].
Nature of the extended components classified according to the geometry derived from the value of Δ: polar (Δ ≤ 30°), equatorial or torus-like (Δ ≥ 60°), and mixed classification (30° < Δ < 60°). Doubtful cases (highlighted in italics) correspond to galaxies where the estimates derived from the MSR and HSR dataset are not in agreement or where the orientation of the outflow axis is uncertain (NGC 4388, NGC 6814, and NGC 7213).
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