Table 2
Patterns of emission in atomic and molecular species.
Source | [O i] | CO 14–13 | H2O 212–101 | OH 84.6 | ||
|
||||||
Compact emission | ||||||
|
||||||
NGC 1333-IRAS2A | ... | x | x | ... | ||
Ced110-IRS4 | x | b | x | x | ||
BHR71 | x | r | ... | ... | ||
L483 | x | x | x | x | ||
L723 | x | b | b | x | ||
L1489 | x | x | x | x | ||
TMR1 | x | x | r | x | ||
TMC1 | x | b | b | x | ||
RNO91 | x | x | r | x | ||
|
||||||
Extended emission | ||||||
|
||||||
NGC 1333-IRAS4A | r | rb | rb | r | ||
NGC 1333-IRAS4B | b | b | b | b | ||
L1527 | r | b | x | x | ||
Ser SMM1 | rb | x | b | b | ||
Ser SMM4 | b | b | ... | ... | ||
Ser SMM3 | rb | rb | rb | b | ||
TMC1A | b | b | rb | b | ||
HH46 | r | x | rb | x | ||
IRAS 15398 | rb | rb | rb | rb |
Notes.Compact emission (see text) is denoted with “x”. Red and blue extended (outflow) emission that accounts for ≥50% of the on-source flux is denoted with “r” and “b”. BHR71 and Ser SMM4 were not observed in the H2O 212–101 and OH 84.6 μm lines. NGC 1333-IRAS2A shows non-detections of the above lines; the CO 15–14 line is used instead of CO 14–13 and the H2O 303–212 line instead of H2O 212–101 line.
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