A Sensitive Very Large Array Search for Small‐Scale Glycine Emission toward OMC‐1

Abstract

We have conducted a deep Q-band (� � 7 mm) search with the Very Large Array (VLA) toward OMC-1 for the lowest energy conformation (conformer I) of glycine (NH2CH2COOH) in four rotational transitions: 615–514 ,6 24–523 ,7 17–616, and 707–606. Our VLA observations sample the smallest scale structures to date in the search for glycine toward OMC-1. No glycine emission features were detected. Thus, if glycine exists in OMC-1, it is below our detection limit, or it is more spatially extended than other large molecules in this source, or it is primarily in its high-energy form (conformer II). Our VLA glycine fractional abundance limits in OMC-1 are comparable to those determined from previous IRAM 30 m measurements—somewhat better or worse depending on the specific source model—and the entire � 1 0 primary beam of the VLA was searched while sensitive to an areal spatial scale � 150 times smaller than the 24 00 beam of the IRAM single-element telescope. In the course of this work, we detected and imaged the 414–313 A and E transitions of methyl formate (HCOOCH3) and also the 202–101 transition of formic acid (HCOOH). Since formic acid is a possible precursor to glycine, our glycine limits and formic acid results provide a constraint on this potential formation chemistry route for glycine in OMC-1. Subject headings: ISM: abundances — ISM: clouds — ISM: individual (OMC-1) — ISM: molecules — radio lines: ISM