ALMA plus IRAM-30m observations of SiO, SiS, and CS toward IRC+10216 show clumpy shells and molecular abundance profiles that support episodic mass loss over the past few hundred years.
H., & Tafalla, M.1993
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IRC+10216 mass loss properties through the study of $\lambda$3mm emission: Large spatial scale distribution of SiO, SiS, and CS
ALMA plus IRAM-30m observations of SiO, SiS, and CS toward IRC+10216 show clumpy shells and molecular abundance profiles that support episodic mass loss over the past few hundred years.