Table 1.
HCG H I sample.
HCG | Nmem | RA | Dec | cz⊙ | Dist. | VLA | Δvchan | σrms | Beam Size | NHI (4σ) |
---|---|---|---|---|---|---|---|---|---|---|
(deg) | (deg) | (km s−1) | (Mpc) | Config. | (km s−1) | (mJy beam−1) | (arcsec) | (cm−2) | ||
2 | 3 | 7.87517 | 8.43126 | 4326 | 50 | D | 10.3 | 0.74 | 69.3 × 51.4 | 1.9 × 1019 |
7 | 4 | 9.84960 | 0.87818 | 4224 | 50 | C,D | 20.6 | 0.3 | 35.0 × 28.0 | 4.0 × 1019 |
10 | 4 | 21.53076 | 34.69095 | 4761 | 50 | DnC | 20.6 | 0.39 | 61.6 × 49.7 | 1.7 × 1019 |
15 | 6 | 31.91244 | 2.13827 | 7042 | 96 | DnC | 20.6 | 0.48 | 60.7 × 47.5 | 2.2 × 1019 |
16 | 5 | 32.38881 | −10.16298 | 3977 | 49 | C,D | 20.6 | 0.41 | 38.9 × 31.7 | 4.3 × 1019 |
19 | 3 | 40.68807 | −12.41181 | 4253 | 53 | C,D | 10.3 | 0.47 | 41.0 × 27.0 | 3.9 × 1019 |
22 | 4 | 45.88027 | −15.67570 | 2626 | 37 | CnB,D | 20.6 | 0.56 | 50.9 × 36.8 | 3.9 × 1019 |
23 | 5 | 46.77701 | −9.58547 | 4921 | 65 | C | 20.6 | 0.54 | 25.3 × 20.0 | 13.9 × 1019 |
25 | 4 | 50.18220 | −1.05192 | 6343 | 82 | DnC | 20.6 | 0.5 | 65.4 × 56.6 | 1.7 × 1019 |
26 | 7 | 50.47584 | −13.64586 | 9618 | 130 | C | 10.3 | 0.63 | 25.5 × 16.8 | 13.5 × 1019 |
30 | 4 | 69.11918 | −2.83239 | 4645 | 61 | DnC | 20.6 | 0.51 | 57.9 × 44.8 | 2.6 × 1019 |
31 | 5 | 75.40372 | −4.25671 | 4068 | 53 | CnB | 10.3 | 0.65 | 14.6 × 12.1 | 33.6 × 1019 |
33 | 4 | 77.69969 | 18.03465 | 7795 | 107 | C | 20.6 | 0.82 | 17.5 × 15.4 | 39.4 × 1019 |
37 | 5 | 138.39859 | 30.01417 | 6741 | 97 | DnC | 20.6 | 0.74 | 49.5 × 47.4 | 4.1 × 1019 |
38 | 3 | 141.91194 | 12.28081 | 8652 | 123 | D | 4.9 | 1.24 | 85.6 × 57.6 | 1.6 × 1019 |
40 | 5 | 144.72717 | −4.85196 | 6628 | 99 | DnC | 20.6 | 0.33 | 58.8 × 44.8 | 1.6 × 1019 |
47 | 4 | 156.45175 | 13.73157 | 9508 | 136 | C,D | 4.9 | 0.49 | 31.0 × 20.0 | 5.0 × 1019 |
48 | 2 | 159.44020 | −27.08746 | 2352 | 34 | DnC | 20.6 | 0.78 | 54.3 × 37.4 | 5.0 × 1019 |
49 | 5 | 164.15204 | 67.17920 | 9939 | 139 | DnC | 10.3 | 0.4 | 47.4 × 37.1 | 2.1 × 1019 |
54 | 5 ( * ) | 172.31364 | 20.57852 | 1412 | 27 | C | 10.3 | 0.46 | 20.8 × 16.9 | 11.9 × 1019 |
56 | 5 | 173.13297 | 52.94860 | 8110 | 116 | C,D | 4.9 | 0.49 | 23.5 × 19.6 | 6.8 × 1019 |
57 | 8 | 174.46054 | 21.98504 | 9032 | 135 | C | 4.9 | 0.62 | 23.7 × 18.9 | 8.8 × 1019 |
58 | 5 | 175.54908 | 10.31703 | 6138 | 85 | DnC,D | 20.6 | 0.25 | 65.8 × 57.0 | 0.9 × 1019 |
59 | 4 | 177.10671 | 12.72623 | 4008 | 60 | C,D | 4.9 | 0.63 | 24.0 × 16.0 | 10.4 × 1019 |
61 | 3 | 183.09972 | 29.17781 | 3956 | 60 | C | 4.9 | 0.35 | 26.2 × 18.8 | 4.6 × 1019 |
62 | 4 | 193.28399 | −9.22410 | 4239 | 60 | C | 4.9 | 0.62 | 24.8 × 14.9 | 10.8 × 1019 |
68 | 5 | 208.42036 | 40.32794 | 2401 | 35 | D | 10.3 | 0.68 | 58.3 × 54.8 | 2.0 × 1019 |
71 | 5 | 212.76906 | 25.48492 | 9199 | 131 | C,D | 4.9 | 0.44 | 26.0 × 20.0 | 5.4 × 1019 |
79 | 4 | 239.80365 | 20.75163 | 4369 | 59 | C | 10.3 | 0.5 | 20.8 × 17.4 | 12.5 × 1019 |
88 | 4 | 313.09503 | −5.75790 | 6032 | 74 | C | 20.6 | 0.3 | 22.6 × 17.2 | 10.1 × 1019 |
90 | 4 | 330.52343 | −31.96680 | 2635 | 33 | DnC | 41.2 | 0.55 | 49.1 × 39.9 | 5.1 × 1019 |
91 | 4 | 332.30172 | −27.77593 | 7195 | 92 | DnC | 20.6 | 0.66 | 51.3 × 47.0 | 3.5 × 1019 |
92 | 4 | 339.00215 | 33.96577 | 6614 | 87 | B,C,D | 20.6 | 0.06 | 15.0 × 15.0 | 3.7 × 1019 |
93 | 4 | 348.85099 | 18.98311 | 5136 | 64 | DnC | 20.6 | 0.4 | 59.7 × 53.3 | 1.6 × 1019 |
95 | 4 | 349.88240 | 9.49185 | 11615 | 153 | CnB | 20.6 | 0.32 | 21.4 × 19.3 | 10.1 × 1019 |
96 | 4 | 351.99291 | 8.77408 | 8725 | 116 | C | 20.6 | 0.21 | 26.9 × 18.3 | 5.4 × 1019 |
97 | 5 | 356.86224 | −2.30542 | 6579 | 85 | DnC | 20.6 | 0.44 | 63.2 × 49.5 | 1.8 × 1019 |
100 | 5 | 0.33654 | 13.13256 | 5461 | 67 | DnC | 20.6 | 0.47 | 58.7 × 50.5 | 2.1 × 1019 |
Notes. Columns: (1) HCG ID number, (2) number of group members considered in this work, (3 and 4) group coordinates (J2000), (5) heliocentric radial velocity (re-calculated as the mean velocity of the group members), (6) group distance calculated via the Cosmicflows-3 model (Tully et al. 2016; Kourkchi et al. 2020), which have uncertainties of ∼3 Mpc, (7) VLA configurations the target group was observed with, (8) channel width, (9) rms noise, (10) synthesised beam size, (11) 4σ column density sensitivity (over 20 km s−1). ( * )The five ‘members’ of HCG 54 are now thought to be clumps all associated with a single merging system.
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