Table 4
KDA-resolved UCHII distances.
| CORNISH name | KDA | Strong H I abs. | d (kpc) |
|---|---|---|---|
| G024.4698+00.4954 | n | 51 | 5.5 ± 0.3 |
| G024.4721+00.4877 | n | 51 | 5.5 ± 0.3 |
| G024.4736+00.4950 | n | 51 | 5.5 ± 0.3 |
| G024.8497+00.0881 | n | 51 | 5.8 ± 0.3 |
| G026.0083+00.1369 | f | 55 | 13.8 ± 0.5 |
| G026.8304−00.2067 | f | 55 | 11.9 ± 0.3 |
| G029.7704+00.2189 | f | 55 | 9.8 ± 0.3 |
| G030.7579+00.2042 | t | 55 | 7.2 ± 0.6 |
| G030.7661−00.0348 | t | 51 | 7.2 ± 0.6 |
| G031.2420−00.1106 | f | 55 | 12.7 ± 0.4 |
| G034.2544+00.1460 | n | 51 | 3.6 ± 0.4 |
| G034.2571+00.1466 | n | 51 | 3.6 ± 0.4 |
| G035.4570−00.1791 | f | 55 | 9.7 ± 0.4 |
| G037.7562+00.5605 | f | 55 | 12.2 ± 0.5 |
| G037.9723−00.0965 | f | 55 | 9.7 ± 0.4 |
| G045.5431−00.0073 | t | 55 | 5.9 ± 0.9 |
| G049.4640−00.3511 | t | 51 | 5.5 ± 2.2 |
| G049.4891−00.3763 | t | 51 | 5.5 ± 2.2 |
| G050.3157+00.6747 | f | 55 | 8.6 ± 0.5 |
| G061.4763+00.0892 | t | 51 | 4.0 ± 1.5 |
| G061.4770+00.0891 | t | 51 | 4.0 ± 1.5 |
Notes. The distances and errors were derived with the Reid et al. (2009) code and the H I E/A method was used to resolve the KDA. The sources that are found at the near, far, and tangent distance, are labelled with n, f, and t, correspondingly. The third column indicates whether the H I spectra usedfor the KDA resolution were of good quality (i.e. mostly in absorption, marked with 51) or poor (i.e. mostly in emission, indicated with 55).
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