Fig. 4

FWHM of the broad velocity component identified in the 12CO J = 10–9 line profiles for each type of YSOs versus their bolometric luminosities. Low-mass Class 0 (LM0) sources are indicated with blue pluses, low-mass Class I (LMI) with black triangles, intermediate-mass (IM) YSOs with green asterisks and high-mass (HM) objects with red crosses. For the high-mass sources, the 12CO J = 3–2 width is used instead. The black dashed line indicates the linear function that fits the relation between the FWHM and the logarithm of Lbol.
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