paper

First detection of ethylene oxide and acetaldehyde in hot core G358.930.03 MM1: Tracing prebiotic oxygen chemistry

arXiv:2509.03382 · doi:10.1016/j.newast.2025.102465

Abstract

Ethylene oxide (c-CHO) and its isomer, acetaldehyde (CHCHO), are important complex organic molecules owing to their potential role in the formation of amino acids (R-CH(NH)-COOH) in ISM. The detection of c-CHO in hot molecular cores suggests that the possible existence of larger ring-shaped molecules containing more than three carbon atoms, such as furan (c-CHO), which shares structural similarities with ribose (CHO5), the sugar component of DNA. In this study, we report the first detection of the rotational emission lines of c-CHO and CHCHO towards the hot molecular core G358.930.03 MM1, based on observations from the Atacama Large Millimeter/Submillimeter Array (ALMA) in band 7. The fractional abundances of c-CHO and CHCHO relative to H are and , respectively. The column density ratio between CHCHO and c-CHO is . A Pearson correlation heat map reveals strong positive correlations ( 0.5) between the abundances and excitation temperatures of c-CHO and CHCHO, suggesting a possible chemical connection between those two molecules. To investigate this further, we conducted a two-phase warm-up chemical model using the gas-grain chemical code UCLCHEM. A comparison between our derived abundances and the predictions from our chemical model and existence model demonstrates good agreement within factors of 0.73 and 0.74, respectively. We propose that c-CHO may form in G358.930.03 MM1 via the grain surface reaction between CH and O, but CHCHO may be produced through the surface reaction between CH and HCO.

Published in New Astronomy

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