Fig. 3

Rotational temperatures of warm (Eup = 14 − 24) CO (top) and H2O (bottom) as function of bolometric luminosity. Orange circles show YSOs from Green et al. (2013), Karska et al. (2013), and Manoj et al. (2013). Dark blue crosses show intermediate-mass YSOs from the WISH program and light blue diamonds high-mass YSOs from Karska et al. (2014a). A few sources with luminosities ~ 102L⊙ shown with orange crosses are from Manoj et al. (2013) and can also be regarded as intermediate-mass YSOs. Uncertainties of the CO and H2O rotational temperatures are shown for L1641 S3 MMS1, which is representative of the sample.
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