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Table 3:

Origin of line emission and cooling rates of various species for the HH 46 central spaxel.
Species Cooling Origin
  10-3 $L_\odot$  
CO 0.1 Passively heated envelope
CO 3.8 UV-heated cavity walls
CO 2.8 C-type shocks
H2O 0.1 Passively heated envelope
H2O 5.0 UV or C-type shocks
O I 9.5 J-type shock
OH >2.4 J-type shock
C II 0.1 Surrounding cloud
Total >23.8  

Source LaTeX | All tables | In the text

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