Table 1
Basic information on the three CMZ molecular clouds.
| CMZ cloud | RA | Dec | l | b | Vlsr | Reff | Tdust | Mass | nH2 |
|---|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss) | (dd:mm:ss) | (deg) | (deg) | (km s−1) | (pc) | (K) | (103 M⊙) | (104 cm−3) | |
| 20 km s−1 | 17:45:37.4 | −29:05:20 | 359.87 | −0.08 | 12.5 | 5.1 | 15.8 | 33.9 | 0.9 |
| Sgr C | 17:44:44.1 | −29:27:46 | 359.45 | −0.11 | −52.6 | 1.7 | 20.6 | 2.5 | 1.8 |
| cloud e | 17:46:45.5 | −28:31:34 | 0.48 | 0.00 | 31.1 | 3.6 | 16.4 | 14.5 | 1.1 |
Notes. The cloud effective radius, total gas mass, and H2 volume density are retrieved from Kauffmann et al. (2017a). The averaged dust temperature is the mean value over a column density threshold of 9 × 1022 cm−2 in the fore/background-subtracted column density map of Battersby et al. (2024).
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