CH lines at 537 GHz. The positions of the fine structure lines are shown shifted by the systemic velocity of the YSOs. The thickness of the three lines indicates the relative theoretical intensities. Where the lines are detected, a Gaussian curve in red is fitted to the strongest transition and its parameters are given in Table B.1. The broad feature in N1333 I4A is an interfering HO line from the other sideband.
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