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Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey

Authors :
R. Fuentetaja
C. Bermúdez
C. Cabezas
M. Agúndez
B. Tercero
N. Marcelino
J. R. Pardo
L. Margulès
R. A. Motiyenko
J.-C. Guillemin
P. de Vicente
J. Cernicharo
Consejo Superior de Investigaciones Científicas [Spain] (CSIC)
Universidad de Valladolid [Valladolid] (UVa)
Instituto Geografico Nacional (IGN)
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 (PhLAM)
Université de Lille-Centre National de la Recherche Scientifique (CNRS)
Institut des Sciences Chimiques de Rennes (ISCR)
Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes)
Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Ecole Nationale Supérieure de Chimie de Rennes (ENSCR)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)
Ministerio de Ciencia e Innovacion of Spain (MICIU) [PID2019-106110GB-I00, ERC-2013-Syg-610256-NANOCOSMOS]
ERC [CONVREC-2021-317]
Ministerio de Universidades [PID2019-107115GB-C21]
[PID2019-106235GB-I00]
Source :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2023, 671, pp.L6. ⟨10.1051/0004-6361/202245732⟩
Publication Year :
2023
Publisher :
EDP Sciences, 2023.

Abstract

We report the detection of methyl ketene towards TMC-1 with the QUIJOTE line survey. Nineteen rotational transitions with rotational quantum numbers ranging from J = 3 up to J = 5 and Ka ≤ 2 were identified in the frequency range 32.0–50.4 GHz, 11 of which arise above the 3σ level. We derived a column density for CH3CHCO of N = 1.5 × 1011 cm−2 and a rotational temperature of 9 K. Hence, the abundance ratio between ketene and methyl ketene, CH2CO/CH3CHCO, is 93. This species is the second C3H4O isomer detected. The other, trans-propenal (CH2CHCHO), corresponds to the most stable isomer and has a column density of N = (2.2 ± 0.3)×1011 cm−2, which results in an abundance ratio CH2CHCHO/CH3CHCO of 1.5. The next non-detected isomer with the lowest energy is cis-propenal, which is therefore a good candidate for future discovery. We have carried out an in-depth study of the possible gas-phase chemical reactions involving methyl ketene to explain the abundance detected, achieving good agreement between chemical models and observations.

Details

ISSN :
14320746 and 00046361
Volume :
671
Database :
OpenAIRE
Journal :
Astronomy & Astrophysics
Accession number :
edsair.doi.dedup.....80efbe373c2e6ed3ad676ef51c20e907
Full Text :
https://doi.org/10.1051/0004-6361/202245732