Table A.3.
Table comparing the predicted H I column densities and H I gas masses to values from the literature.
# | Galaxy | log MH I
![]() |
log MH I
![]() |
log N(H I)max, pred | log N(H I)min, pred | log N(H I)obs |
---|---|---|---|---|---|---|
1 | Haro2 | 8.37![]() |
8.58![]() |
19.47 | 18.79 | 19.6–20.52 |
2 | Haro3 | 7.93![]() |
9.05![]() |
18.92 | 18.29 | |
3 | Haro11 | 9.75![]() |
8.70![]() |
19.08 | 18.73 | |
4 | He2-10 | 7.56![]() |
8.49![]() |
19.33 | 18.74 | |
5 | HS0052+2536 | 9.79![]() |
< 10.68 | 20.0 | 18.54 | |
6 | HS0822+3542 | 4.94![]() |
7.75![]() |
21.67 | 21.67 | |
7 | HS1222+3741 | 8.39![]() |
20.16 | 20.16 | ||
8 | HS1304+3529 | 8.83![]() |
20.42 | 20.42 | ||
9 | HS1319+3224 | 6.4![]() |
18.46 | 17.86 | ||
10 | HS1330+3651 | 8.43![]() |
20.37 | 20.37 | ||
11 | HS1442+4250 | 5.48![]() |
8.49![]() |
20.84 | 19.29 | |
12 | IIZw40 | 8.52![]() |
8.75![]() |
19.18 | 18.96 | |
13 | IZw18 | 7.68![]() |
8.0![]() |
20.27 | 19.12 | 21.0–21.52; 21.28±0.033 |
14 | Mrk153 | 8.56![]() |
< 8.84 | 19.61 | 18.4 | |
15 | Mrk209 | 6.87![]() |
7.44![]() |
19.87 | 18.59 | |
16 | Mrk930 | 9.62![]() |
9.5![]() |
19.54 | 19.54 | |
17 | Mrk1089 | 9.39![]() |
10.17![]() |
18.96 | 18.33 | |
18 | Mrk1450 | 7.49![]() |
7.63![]() |
19.27 | 18.81 | |
19 | NGC1140 | 8.01![]() |
9.54![]() |
18.43 | 18.28 | |
20 | NGC1569 | 8.47![]() |
8.25![]() |
19.26 | 18.98 | |
21 | NGC1705 | 6.63![]() |
7.88![]() |
19.1 | 17.97 | |
22 | NGC5253 | 7.85![]() |
8.03![]() |
18.83 | 18.79 | |
23 | NGC625 | 5.46![]() |
8.04![]() |
19.16 | 18.72 | |
24 | Pox186 | 5.3![]() |
< 6.30 | 19.75 | 19.3 | |
25 | SBS0335-052 | 8.72![]() |
8.64![]() |
21.29 | 18.85 | 21.4–21.72; 21.7±0.053 |
26 | SBS1159+545 | 8.22![]() |
< 7.80 | 21.04 | 20.13 | |
27 | SBS1211+540 | 6.69![]() |
7.75![]() |
20.56 | 20.56 | |
28 | SBS1249+493 | 8.41![]() |
9.0![]() |
20.11 | 19.65 | |
29 | SBS1415+437 | 7.79![]() |
8.64![]() |
20.8 | 20.8 | |
30 | SBS1533+574 | 8.74![]() |
9.48![]() |
19.57 | 19.08 | |
31 | Tol1214-277 | 2.41![]() |
< 8.51 | 19.93 | 19.93 | |
32 | UM448 | 8.26![]() |
9.78![]() |
19.26 | 18.68 | |
33 | UM461 | 7.07![]() |
7.86![]() |
20.01 | 19.48 | |
34 | VIIZw403 | 6.06![]() |
7.51![]() |
19.88 | 19.61 | |
35 | UGC4483 | 6.0![]() |
7.40![]() |
20.44 | 19.42 | |
36 | UM133 | 8.01![]() |
8.33![]() |
20.38 | 20.38 | |
37 | HS0017+1055 | 7.66![]() |
< 8.24 | 20.43 | 20.43 | |
38 | HS2352+2733 | 4.53![]() |
< 10.36 | 18.77 | 18.77 | |
39 | NGC4214-c | 7.17![]() |
< 8.58 | 18.95 | 17.43 | 21.12±0.033 |
40 | NGC4214-s | 6.61![]() |
< 8.58 | 19.02 | 18.34 | 21.12±0.033 |
This table complements the discussion from Sect. 7.2.2 and the H I gas mass comparison presented in Fig. A.2. (0): The interval is the highest density interval at 94%. (1): Rémy-Ruyer et al. (2014) (2): Kunth et al. (1998) (3): James et al. (2014)
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