Fig. 17
A comparison of 12CO emission from the broad component of HH 100 IRS (black circles), DR Tau (blue diamonds), and TW Hya (red squares). The emission in 12CO v = 1−0 is very similar for HH 100 IRS and the CTTS DR Tau, with much weaker emission seen from the older CTTS TW Hya. CO v = 2−1 emission is stronger from HH 100 IRS than DR Tau.
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