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Water in star-forming regions with Herschel (WISH): III. Far-infrared cooling lines in low-mass young stellar objects

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Academic year: 2021

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Fig. 5. Extent of line emission along the outflow direction for the selected molecular and atomic lines
Fig. 4. The same as Figure 3 but for the Class I source L1489.
Fig. 8. Relative contributions of CO (red), [O i ] (green), OH (yel- (yel-low) and H 2 O (blue) to the total far-IR gas cooling integrated over the entire PACS array are shown from left to right hori-zontally for each source
Table 3. CO and H 2 O rotational excitation and number of emitting molecules N u based on the full array data.
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