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Table 4
Absolute and relative luminosities of CO and H2O for the three physical components in each source.
Component | IRAS2A | HH 46 | DK Cha | |||
for CO | 10-3 L⊙ | % | 10-3 L⊙ | % | 10-3 L⊙ | % |
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passive | 0.3 | 7 | 0.5 | 7 | 0.1 | 2 |
UV | 0.8 | 20 | 3.1 | 45 | 4.0 | 78 |
C-shocks | 3.0 | 73 | 3.3 | 48 | 1.0 | 20 |
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total | 4.1 | 100 | 6.9 | 100 | 5.1 | 100 |
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Component | IRAS2A | HH 46 | DK Cha | |||
for H2O | 10-3 L⊙ | % | 10-3 L⊙ | % | 10-3 L⊙ | % |
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passive | 0.02 | 0.02 | 0.53 | 0.38 | 0.05 | 0.17 |
UV | 0.001 | 0.001 | 0.04 | 0.03 | 3(−5) | 1(−4) |
C-shocks | 100 | >99.9 | 140 | 99.6 | 30 | 99.8 |
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total | 100 | 100 | 140 | 100 | 30 | 100 |
Notes. The tabulated values are for the adopted source inclinations of 90, 53 and 0° (Table 2). They do not represent the total line cooling budget, which would require integrating over all inclinations from edge-on to pole-on.
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