Complex molecules toward low-mass protostars: the Serpens core
Karin I. Oberg, Nienke van der Marel, Lars E. Kristensen, Ewine F. van, Dishoeck

TL;DR
This study detects and analyzes complex organic molecules in the Serpens core's low-mass protostars, revealing similar abundance levels to high-mass hot cores and insights into ice photochemistry processes.
Contribution
First detection of complex organic molecules in multiple low-mass protostars within the Serpens core, expanding understanding of astrochemistry in low-mass star-forming regions.
Findings
Complex organics detected in all sources with narrow lines.
Abundances vary by an order of magnitude, highest in SMM1.
HCOOCH3 is relatively more abundant in low-mass protostars.
Abstract
Gas-phase complex organic molecules are commonly detected toward high-mass protostellar hot cores. Detections toward low-mass protostars and outflows are comparatively rare, and a larger sample is key to investigate how the chemistry responds to its environment. Guided by the prediction that complex organic molecules form in CH3OH-rich ices and thermally or non-thermally evaporate with CH3OH, we have identified three sight-lines in the Serpens core - SMM1, SMM4 and SMM4-W - which are likely to be rich in complex organics. Using the IRAM 30m telescope, narrow lines (FWHM of 1-2 km s-1) of CH3CHO and CH3OCH3 are detected toward all sources, HCOOCH3 toward SMM1 and SMM4-W, and C2H5OH not at all. Beam-averaged abundances of individual complex organics range between 0.6 and 10% with respect to CH3OH when the CH3OH rotational temperature is applied. The summed complex organic abundances also…
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