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Table A.1.
H I emission lines and Gaussian fits.
| MW line | MB line | |
|---|---|---|
| Peak - TA [K] | ||
| 1st | 11.1 | 2.2 |
| 2nd | 4.4 | 1.7 |
| 3rd | 4.4 | 1.3 |
| 4th | 3.7 | 0.7 |
| Center [km s−1] | ||
| 1st | 2.4 | 239.8 |
| 2nd | 7.3 | 219.1 |
| 3rd | -2.2 | 219.6 |
| 4th | -1.6 | 228.3 |
| Width - σ [km s−1] | ||
| 1st | 2.2 | 18.4 |
| 2st | 2.8 | 10.3 |
| 3nd | 3.8 | 4.9 |
| 4th | 9.6 | 2.3 |
Notes. HI4PI Gaussian fits results (see Fig.1) toward J0332-7249 by Kalberla & Haud (2018). The uncertainties in peak brightness, TA, and line width, σ, correspond to the inherent calibration uncertainties of about 5% (HI4PI Collaboration 2016), in ΔvLSR ≤ 1.28 km s−1.
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