Table 1.
Details of the galaxies with gas.
| Galaxy | Class | r | Mgas | E(B − V) | n° | PAg | PAs | PAp | ΔPAgs | ΔPAgp |
|---|---|---|---|---|---|---|---|---|---|---|
| [105 M⊙] | [mag] | [°] | [°] | [°] | [°] | [°] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| PGC 015524 | 1 | 50 | 29.0 | 0.1321 | 2 | 25.7 ± 3.0 | 116.5 ± 12.6 | 172.9 ± 7.5 | 90.8 | 147.2 |
| PGC 046860 | 3 | 49 | 0.2(*) | 0.0566 | 1 | (…) | 56.0 ± 1.8 | 57.6 ± 1.0 | (…) | (…) |
| PGC 047177 | 3 | 226 | 6.7 | 0.0542 | 2 | 107.4 ± 2.3 | 95.3 ± 2.0 | 98.4 ± 1.3 | 12.1 | 9.0 |
| PGC 047197 | 3 | 226 | 0.1(*) | 0.0501 | 1 | (…) | 24.2 ± 29.7 | 118.4 ± 2.1 | Aligned | ∼90 |
| PGC 047202 | 2 | 226 | 4.5 | 0.0503 | 1 | (…) | 166.4 ± 2.8 | 172.2 ± 2.5 | (…) | (…) |
| PGC 047273 | 3 | 226 | 6.5 | 0.0502 | 1 | 28.7 ± 2.3 | 96.8 ± 2.3 | 93.6 ± 2.2 | 68.1 | 64.9 |
| PGC 047590 | 3 | 129 | 1.0 | 0.0549 | 1 | 102.9 ± 3.8 | 46.9 ± 29.7 | 132.4 ± 3.8 | 56.0 | 29.5 |
| PGC 049940 | 1 | 41 | 3.9 | 0.0663 | 3 | 54.4 ± 0.8 | 51.4 ± 9.1 | 51.7 ± 1.9 | 3.0 | 2.7 |
| PGC 065588 | 1 | 66 | 1.3 | 0.0333 | 1 | 102.9 ± 0.8 | 136.1 ± 2.3 | 62.1 ± 1.1 | 33.2 | 40.8 |
| PGC 073000 | 1 | 66 | 44.8 | 0.0145 | 3 | 43.9 ± 2.3 | 66.6 ± 5.0 | 160.8 ± 0.3 | 22.7 | 116.9 |
| PGC 097958 | 3 | 226 | 0.5(*) | 0.0649 | 1 | (…) | 45.4 ± 1.5 | 47.3 ± 0.3 | Aligned | ∼0 |
Notes. Column (1): Galaxy name. Column (2): 1 = BCG, 2 = BCG in the SSC, 3 = “satellite” in the SSC. Column (3): Richness of the cluster from Laine et al. (2003). Column (4): Mass of the gas from Hα flux. Values with (*) are upper limits. Column (5): Foreground Galactic extinction from Schlegel et al. (1998). Column (6): Number of Gaussian components employed to model the emission lines. Column (7): Gas kinematic position angle. Column (8): Stellar kinematic position angle from Krajnović et al. (2018). Column (9): PA of the isophotal major axis from Krajnović et al. (2018). Column (10): Absolute difference between Cols. 6 and 7. Aligned = From a visual inspection, PAg is nearly aligned to PAs. Column (11): Absolute difference between Cols. 6 and 8. For those galaxies with the “aligned” keyword in Col.(9), we report a rough estimation.
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