Table 2
Environmental properties of the HALOGAS sample galaxies.
| Galaxy | # Group | NOGG | L B, group | R group | v min, group | v max, group | LB/LB, group | LB/LB, max | R/Rgroup | v |
| ID | members | number | [1010 M⊙] | [Mpc] | [km s-1] | [km s-1] | [km s-1] | |||
|
|
||||||||||
| NGC 0672 | 2 | 88 | 1.3 | 0.01 | –52 | 29 | 0.64 | 1.00 | 0.55 | 29 |
| NGC 0891a | − | − | − | − | − | − | − | − | − | − |
| NGC 0925 | 6 | 149 | 3.1 | 0.56 | –16 | 47 | 0.69 | 1.00 | 0.25 | –16 |
| NGC 0949 | 6 | 149 | 3.1 | 0.56 | –16 | 47 | 0.15 | 0.21 | 1.00 | 47 |
| UGC 2082b | − | − | − | − | − | − | − | − | − | − |
| NGC 1003a | − | − | − | − | − | − | − | − | − | − |
| NGC 2403 | 2 | 319 | 1.8 | 0.24 | –14 | 1 | 0.88 | 1.00 | 0.13 | 1 |
| UGC 4278 | 6 | 345 | 1.4 | 0.77 | –90 | 35 | 0.30 | 1.00 | 0.44 | 21 |
| NGC 2541 | 6 | 345 | 1.4 | 0.77 | –90 | 35 | 0.24 | 0.79 | 0.21 | 35 |
| NGC 3198 | 2 | 462 | 1.7 | 0.43 | –25 | 1 | 0.96 | 1.00 | 0.05 | 1 |
| NGC 4062 | 27 | 631c | 21.0 | 1.27 | –163 | 525 | 0.03 | 0.07 | 0.86 | 45 |
| NGC 4244 | 16 | 636 | 3.1 | 0.80 | –93 | 83 | 0.22 | 0.66 | 0.31 | –42 |
| NGC 4258 | 21 | 644 | 9.0 | 1.07 | –103 | 160 | 0.51 | 1.00 | 0.24 | –40 |
| NGC 4274 | 27 | 631c | 21.0 | 1.27 | –163 | 525 | 0.04 | 0.10 | 0.45 | 194 |
| NGC 4414 | 27 | 631c | 21.0 | 1.27 | –163 | 525 | 0.05 | 0.13 | 0.21 | –3 |
| NGC 4448 | 27 | 631c | 21.0 | 1.27 | –163 | 525 | 0.02 | 0.06 | 0.37 | –79 |
| NGC 4559 | 27 | 631c | 21.0 | 1.27 | –163 | 525 | 0.12 | 0.30 | 0.42 | 79 |
| NGC 4565 | 3 | 648 | 14.9 | 0.26 | –18 | 107 | 0.78 | 1.00 | 0.25 | –18 |
| UGC 7774 | 21 | 644 | 9.0 | 1.07 | –103 | 160 | 0.01 | 0.01 | 0.74 | 3 |
| NGC 4631 | 27 | 631c | 21.0 | 1.27 | –163 | 525 | 0.40 | 1.00 | 0.30 | –91 |
| NGC 5023 | 7 | 723 | 8.0 | 0.45 | –94 | 131 | 0.04 | 0.09 | 0.68 | –77 |
| NGC 5055 | 7 | 723 | 8.0 | 0.45 | –94 | 131 | 0.37 | 0.79 | 1.00 | 8 |
| NGC 5229 | 7 | 723 | 8.0 | 0.45 | –94 | 131 | 0.01 | 0.02 | 0.97 | –94 |
| NGC 5585 | 8 | 766 | 3.1 | 0.54 | 107 | 75 | 0.07 | 0.09 | 0.52 | 75 |
Notes.
(a)
Not included in the Giuricin et al. (2000) catalog due to low galactic latitude.
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