C<sub>3</sub>H<sub>8</sub>O<sub>2</sub> Isomers: Insights into Potential Interstellar Species

2-Methoxyethanol, with a formula C<sub>3</sub>H<sub>8</sub>O<sub>2,</sub> was recently identified in the massive protocluster NGC 6334I. However, its structural isomers, 1,2-propanediol and 1,3-propanediol, remain undetected despite extensive searches in the Sgr B2 region. In this study, we explored the potential energy surface of the C<sub>3</sub>H<sub>8</sub>O<sub>2</sub> system using CCSD(T)/aug-cc-pVTZ//MP2/aug-cc-pVTZ calculations, identifying 11 species, with the geminal diols 2,2-propanediol and 1,1-propanediol as the most stable forms. We examined the gas-phase decomposition barrier of these geminal diols and found that 1,1-propanediol is thermodynamically stable at low temperatures (10-150 K). C<sub>3</sub>H<sub>8</sub>O<sub>2</sub> isomers with energies below 30 kcal/mol are relevant to the ISM, as they have been identified or tentatively detected in irradiation experiments of ice analogs of CO, H<sub>2</sub>O, and CH<sub>3</sub>OH.

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Publication Details

Journal
The Journal of Physical Chemistry A
Published
2024-11-11
DOI
https://doi.org/10.1021/acs.jpca.4c04804
Citations
5
Primary Topic
Molecular Spectroscopy and Structure
Type
article
Field-Weighted Citation Impact
1.20

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article

C3H8O2 Isomers: Insights into Potential Interstellar Species

Filiberto Ortíz‐Chi, Gabriel Merino, Alan Quintal, Lisset Noriega et al.
5 citations
The Journal of Physical Chemistry A
Molecular Spectroscopy and Structure
1.20
article

C3H8O2 Isomers: Insights into Potential Interstellar Species

Filiberto Ortíz‐Chi, Gabriel Merino, Alan Quintal, Lisset Noriega, Sandra I. Ramírez, Luis Armando González-Ortiz
article en
5 citations

Abstract

2-Methoxyethanol, with a formula C<sub>3</sub>H<sub>8</sub>O<sub>2,</sub> was recently identified in the massive protocluster NGC 6334I. However, its structural isomers, 1,2-propanediol and 1,3-propanediol, remain undetected despite extensive searches in the Sgr B2 region. In this study, we explored the potential energy surface of the C<sub>3</sub>H<sub>8</sub>O<sub>2</sub> system using CCSD(T)/aug-cc-pVTZ//MP2/aug-cc-pVTZ calculations, identifying 11 species, with the geminal diols 2,2-propanediol and 1,1-propanediol as the most stable forms. We examined the gas-phase decomposition barrier of these geminal diols and found that 1,1-propanediol is thermodynamically stable at low temperatures (10-150 K). C<sub>3</sub>H<sub>8</sub>O<sub>2</sub> isomers with energies below 30 kcal/mol are relevant to the ISM, as they have been identified or tentatively detected in irradiation experiments of ice analogs of CO, H<sub>2</sub>O, and CH<sub>3</sub>OH.

The Journal of Physical Chemistry AVol. 128(46)
Universidad Marista de Mérida (MX), Instituto Politécnico Nacional (MX), Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional (MX), Universidad Autónoma del Estado de Morelos (MX)
Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional
Life below water
Openalex Percentile: Top 23%
Molecular Spectroscopy and Structure
1.20
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