Table 4
Atomic and molecular far-IR line luminosities based on the full array data.
| Source | LCO | LH2O | LOH | LOI | LFIR | |||||||||
|
|
||||||||||||||
| NGC 1333-I2A | 3.9 | 7.1 | ... | 1.6 | 12.6 | |||||||||
| NGC 1333-I4A | 13.2 | 20.0 | 1.7 | 0.5 | 35.4 | |||||||||
| NGC 1333-I4B | 22.5 | 27.6 | 5 | 0.3 | 54.1 | |||||||||
| L1527 | 0.3 | 0.5 | 0.3 | 0.8 | 1.9 | |||||||||
| Ced110-IRS4 | 0.1 | 0.1 | 0.2 | 0.5 | 0.9 | |||||||||
| BHR71 | 12.1 | 7.1 | ... | 2.8 | 22.0 | |||||||||
| IRAS 15398 | 2.0 | 0.9 | 0.3 | 1.1 | 4.3 | |||||||||
| L483 | 1.7 | 2.8 | 1.0 | 1.1 | 6.7 | |||||||||
| Ser SMM1 | 42.8 | 23.6 | 11.5 | 14.3 | 93.1 | |||||||||
| Ser SMM4 | 7.4 | 3.6 | ... | 4.2 | 15.2 | |||||||||
| Ser SMM3 | 10.5 | 9.5 | 1.4 | 3.9 | 25.3 | |||||||||
| L723 | 1.9 | 1.2 | 0.6 | 1.0 | 4.7 | |||||||||
|
|
||||||||||||||
| L1489 | 0.7 | 0.8 | 0.5 | 0.4 | 2.4 | |||||||||
| TMR1 | 1.0 | 0.6 | 0.5 | 0.5 | 2.6 | |||||||||
| TMC1A | 0.5 | ... | 0.1 | 0.6 | 1.2 | |||||||||
| TMC1 | 0.5 | 0.3 | 0.5 | 0.9 | 2.2 | |||||||||
| HH46 | 5.8 | 3.8 | 4.1 | 22.8 | 36.5 | |||||||||
| RNO91 | 0.1 | 0.1 | 0.1 | 0.5 | 0.8 | |||||||||
Notes.All luminosities are in 10-3L⊙. Typical uncertainties are better than 30% of the quoted values. BHR71 and Ser SMM4 were not observed in the OH lines in our program, thus their OH luminosities are not available. OH is not detected in NGC 1333-I2A and H2O is not detected in TMC1A.
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