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
References in corpus (18)
- CASA, the Common Astronomy Software Applications for Radio Astronomy
- Complex Chemistry in Star-Forming Regions: An Expanded Gas-Grain Warm-up Chemical Model
- The largest oxigen bearing organic molecule repository
- UCLCHEM: A Gas-Grain Chemical Code
- Ethylene oxide and Acetaldehyde in hot cores
- Identification of interstellar amino acetonitrile in the hot molecular core G10.47+0.03: Possible glycine survey candidate for the future
- Rotational spectroscopy of mono-deuterated oxirane (-CHDO) and its detection towards IRAS 162932422 B
- Identification of the simplest sugar-like molecule glycolaldehyde towards the hot molecular core G358.93-0.03 MM1
- Detection of interstellar cyanamide (NHCN) towards the hot molecular core G10.47+0.03
- Millimetre and sub-millimetre spectroscopy of doubly deuterated acetaldehyde (CHD2CHO) and first detection towards IRAS 16293-2422
- First Identification and Chemical Modeling of New Thiol (SH) Bearing Molecule in the Interstellar Medium: Dithioformic Acid
- A spectral survey of CH3CCH in the Hot Molecular Core G331.512-0.103
- Identification of interstellar cyanamide towards the hot molecular core G358.93-0.03 MM1
- Detection of possible glycine precursor molecule methylamine towards the hot molecular core G358.930.03 MM1
- Detection of antifreeze molecule ethylene glycol in the hot molecular core G358.930.03 MM1
- Observation of Complex Organic Molecules Containing Peptide-like Bonds Toward Hot Core G358.930.03 MM1
- Study of Complex Nitrogen and Oxygen-bearing Molecules toward the High-mass Protostar IRAS 180891732
- Detection and prebiotic chemistry of possible glycine precursor molecule methylenimine towards the hot molecular core G10.47+0.03