Table 3
Averaged rms value in 0.27 km s-1 bin and mean (dash) values of the FWHMb and FWZI for the three water lines and the 12CO J = 10–9 spectra for each sub-type of YSO.
| H2O | 202–111 | 211–202 | 312–303 | 12CO J = 10–9 | 12CO/H2O | |||||||
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FWHM b | FWZI | |
| (km s-1) | (mK) | (km s-1) | (mK) | (km s-1) | (mK) | (km s-1) | (km s-1) | (mK) | (km s-1) | |||
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| LM0 | 30 ± 12 | 23 | 86 ± 45 | 20 | 87 ± 47 | 17 | 86 ± 31 | 20 ± 9 | 112 | 36 ± 14 | 0.7 ± 0.3 | 0.5 ± 0.2 |
| LMI | 18 ± 5 | 22 | 34 ± 13 | 17 | 33 ± 15 | 9 | 42a | 11 ± 1 | 115 | 24 ± 8 | 0.6 ± 0.1 | 0.8 ± 0.4 |
| IM | 29 ± 5 | 24 | 69 ± 19 | 22 | 63 ± 30 | 19 | 79a | 20 ± 4 | 105 | 63 ± 21 | 0.7 ± 0.2 | 0.9 ± 0.1 |
| HM | 27 ± 10 | 78 | 47 ± 10 | 68 | 70 ± 32 | 45 | 71 ± 35 | 22a | 180 | 81 ± 30b | 0.9a | 1.9 ± 0.2b |
Notes. The averaged FWHMb and FWZI ratios calculated from the 12CO and H2O observations are also indicated in the last two columns. LM0: low-mass Class 0 protostars; LMI: low-mass Class I sources; IM: intermediate-mass YSOs; HM: high-mass objects. See specification in the FWZI calculation for the low-mass objects in Mottram et al. 2014.
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