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. 2006 Aug 7;103(33):12274–12279. doi: 10.1073/pnas.0602277103

Fig. 3.

Fig. 3.

Observations of spectral lines toward the carbon-rich shell of IRC+10216 (Upper and Inset) and the oxygen-rich envelope of VYCMa (Lower) at 245 GHz, measured with the SMT telescope of the Arizona Radio Observatory with an Atacama Large Millimeter Array Band 6 mixer.