Table 5
Properties of the ATLASGAL CSC clumps.
| ATLASGAL | v lsr | δv | d | M clump | M vir | SDG | 12CO | MSF | ATLASGAL |
| clump | ( km s-1) | ( km s-1) | (kpc) | (102M⊙) | (102M⊙) | cloud | GMC | assoc. | group |
|
|
|||||||||
| AGAL340.119−00.022 | -121.9 | 2.2 | 6.7 | 16.3 | 3.6 | 15 | 3KPC3 | MMB | G340.256−00.059 |
| AGAL340.182−00.047 | -123.7 | 5.3 | 6.7 | 13.8 | 21.4 | 15 | 3KPC3 | MMB | G340.256−00.059 |
| AGAL340.249−00.046 | -121.3 | 5.3 | 6.7 | 76.0 | 53.1 | 15 | 3KPC3 | MMB/HII | G340.256−00.059 |
| AGAL340.359+00.129 | -119.0 | 3.3 | 6.6 | 3.4 | 3.3 | 88 | 3KPC3 | HII | – |
| AGAL340.784−00.097 | -101.4 | 3.9 | 6.0 | 20.0 | 11.7 | 116 | NORM7.4 | MMB | – |
| AGAL340.508−00.442 | -90.5 | 2.8 | 5.6 | 18.8 | 3.8 | 147 | NORM7.2 | – | G340.556−00.402 |
| AGAL340.466−00.299 | -89.3 | 2.6 | 5.7 | 5.9 | 3.7 | 154 | NORM7.2 | HII | – |
| AGAL340.054−00.244 | -53.0 | 8.8 | 3.8 | 43.0 | 87.8 | 234 | NCEN25 | MMB/YSO/HII | G340.249−00.266 |
| AGAL340.248−00.374 | -50.4 | 5.4 | 3.8 | 48.5 | 37.8 | 298 | NCEN25 | MMB/HII | G340.249−00.266 |
| AGAL340.536−00.152 | -46.7 | 3.8 | 3.7 | 8.6 | 11.9 | 331 | NCEN25 | MMB | G340.529−00.147 |
| AGAL340.656−00.236 | -21.7 | 4.2 | 2.1 | 0.4 | 1.7 | -1 | – | MMB | – |
Notes. Only a small portion of the data is provided here, the full table is available in electronic form at the CDS. Column 1 gives the CSC name. Columns 2 and 3 give the adopted vlsr and the 13CO(2−1) FWHM line-width. Column 4 gives the distance assigned to the clump. Column 5 is the clump mass, derived from the integrated 870 μm flux density. Column 6 is the virial mass, computed as 5δv2R/G. Columns 7 and 8 list associations with SCIMES clouds (Sect. 4 and Table A.1), and with 12CO clouds from García et al. (2014), respectively. Column 9 indicates matches with HMSF tracers (MMB: methanol maser; HII: compact Hii region; YSO: massive young stellar object). Column 10 indicates the ATLASGAL CSC group (see Table 4) to which each clump is associated, if any.
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