Free Access

Fig. 2

thumbnail

PACS line scan OH spectra of the low-mass class 0 young stellar objects in our sample. The x-axis is wavelengths in μm, the y-axis is continuum subtracted flux density in Jy (plus a constant offset). The red dashed lines indicate the rest frequencies of the OH transitions. The blue dotted line represents the rest frequency of CO(31–30), which is blended with OH at 84.42 μm. The sampling of range scans (Ser SMM1 and NGC 1333 IRAS 2A) is different from line scans.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.