Proc. IAU volume 13, issue S332, P249-253 2017 DOI: 10.1017/s174392131700967x View full text
Łukasz Tychoniec, Charles L. H. Hull, John J. Tobin, Ewine F. van Dishoeck

Abstract: The youngest low-mass protostars are known to be chemically rich, accreting matter most vigorously, and producing the most powerful outflows. Molecules are unique tracers of these phenomena. We use ALMA to study several outflow sources in the Serpens Main region. The most luminous source, Ser-SMM1, shows the richest chemical composition, but some complex molecules are also present in S68N. No emission from complex organics is detected toward Seremb 8N, which is the least luminous in the sample. We discuss whe…

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