Table 2.
H I properties of dwarfs measured from the 66″ MFS H I cube.
| Name | RA (J2000) | Dec (J2000) | Integrated flux | vsys | w20 | Disturbed |
|---|---|---|---|---|---|---|
| (hms) | (dms) | (Jy km s−1) | (km s−1) | (km s−1) | ||
| NGC 1437A | 03:43:02.42 | −36:16:24.2 | 7.25 ± 0.7 | 886 | 128 | Y |
| ESO 358−G015 | 03:33:07.06 | −34:48:21.2 | 1.50 ± 0.2 | 1388 | 133 | Y |
| ESO 358−G016 | 03:33:09.19 | −35:43:05.2 | 1.26 ± 0.1 | 1700 | 131 | Y |
| ESO 358−G060 | 03:45:12.29 | −35:34:15.2 | 11.99 ± 1.2 | 803 | 129 | Y |
| ESO 358−G064 | 03:46:28.51 | −36:54:21.6 | 5.59 ± 0.7 | 1465 | 171 | N |
| FCC 090 | 03:31:08.28 | −36:17:24.4 | 0.59 ± 0.07 | 1825 | 129 | N |
| FCC 102 | 03:32:10.56 | −36:13:10.6 | 1.19 ± 0.1 | 1640 | 83 | Y |
| FCC 120 | 03:33:34.18 | −36:36:20.1 | 1.08 ± 0.1 | 846 | 60 | Y |
| FCC 128 | 03:34:07.03 | −36:27:57.6 | 0.14 ± 0.02 | 1543 | 68 | N |
| FCC 134 | 03:34:21.70 | −34:35:33.0 | 0.02 ± 0.01 | 1398 | 34 | N |
| FCC 207 | 03:38:19.25 | −35:07:44.8 | 0.0065 ± 0.006 | 1420 | 38 | N |
| FCC 248 | 03:40:43.37 | −35:51:38.9 | 0.010 ± 0.006 | 1859 | 15 | N |
| FCC 299 | 03:44:58.61 | −36:53:41.6 | 0.31 ± 0.04 | 2100 | 136 | N |
| FCC 306 | 03:45:45.38 | −36:20:46.0 | 2.03 ± 0.1 | 886 | 176 | Y |
| FCC 323 | 03:47:37.46 | −36:21:48.6 | 0.43 ± 0.05 | 1499 | 67 | N |
| FCC B905 | 03:33:57.34 | −34:36:43.2 | 0.52 ± 0.06 | 1248 | 99 | Y |
| FDS6 100b | 03:41:27.84 | −35:43:13.1 | 0.14 ± 0.03 | 1983 | 50 | N |
Notes. The position, integrated flux, and w20 are from the SoFiA catalogue, while vsys is estimated from where 11″ H I iso-velocity intercepts the optical centre. The uncertainty in the integrated flux is a combination of the statistical error and 10% uncertainty in the calibration of the flux scale (Serra et al. 2023).
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