Table B.2
Line parameters of CH3OH
| ID | Source | RA | DEC | Distance | θsource | PA | CH3OH | ||
|---|---|---|---|---|---|---|---|---|---|
| h m s | ° ′ ″ | kpc | ″ | ° | Ipeak K km s−1 | Iintegrated K km s−1 arcsec2 | N × 1016 cm−2 | ||
| 1 | I08303-4303 | 08:32:08.68 | -43:13:45.78 | 2.3 | 1.26±0.12 | 168±42 | 34.30 ± 1.20 | 134.24 ± 7.04 | 414.00±14.00 |
| 2 | I08470-4243 | 08:48:47.79 | -42:54:27.90 | 2.1 | 0.56±0.04 | 113±21 | 86.50 ± 1.10 | 215.68 ± 4.48 | 1040.00±10.00 |
| 3 | I09018-4816 | 09:03:33.46 | -48:28:01.69 | 2.6 | 0.93±0.36 | 10±27 | 32.20 ± 1.60 | 113.28 ± 8.32 | 388.00±19.00 |
| 4 | I10365-5803N | 10:38:32.16 | -58:19:08.43 | 2.4 | 0.98±0.25 | 54±76 | 8.58 ± 0.25 | 55.68 ± 2.56 | 103.00±3.00 |
| 5 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
Notes. The entire version in a machine-readable format is available at the CDS. Column 1 lists the ID number. Column 2 provides the names of the hot core candidates, with a superscript ‘N’ indicating the hot core candidates newly identified in this work. Columns 3 to 7 contain the parameters of the hot core candidates, including peak position, distance from the Sun, deconvolved size, and position angle. The distances from the Sun are compiled in Liu et al. (2020b). The peak positions, sizes, and position angles of the hot core candidates are derived from 2D Gaussian fitting of the CH3OH integrated intensity maps. Columns 8 to 10 present the peak fluxes, integrated fluxes, and column densities.
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