Issue |
A&A
Volume 697, May 2025
|
|
---|---|---|
Article Number | A82 | |
Number of page(s) | 8 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202554343 | |
Published online | 12 May 2025 |
A search for the three isomers of cyano-1,3-butadiene in TMC-1: Implications for bottom-up routes involving 1,3-butadiene⋆
1
Instituto de Física Fundamental, CSIC,
Calle Serrano 123,
28006
Madrid,
Spain
2
Observatorio Astronómico Nacional, IGN,
Calle Alfonso XII 3,
28014
Madrid,
Spain
3
Observatorio de Yebes, IGN,
Cerro de la Palera s/n,
19141
Yebes, Guadalajara,
Spain
★★ Corresponding authors: marcelino.agundez@csic.es; jose.cernicharo@csic.es
Received:
1
March
2025
Accepted:
28
March
2025
The molecule 1,3-butadiene (CH2CHCHCH2) could play a key role in the synthesis of the cyclic molecules cyclopentadiene and benzene in cold dense clouds. Since 1,3-butadiene is non-polar, we searched for its cyano derivative, which exists in the form of three different polar isomers, in the cold dense cloud TMC-1. We used the most recent data obtained with the Yebes 40 m telescope in the Q band (31.0−50.3 GHz) in the frame of the QUIJOTE project. We did not detect either of the isomers of 1-cyano-1,3-butadiene, and we derive 3 σ upper limits to their column densities of 1.2 × 1010 cm−2 and 2.0 × 1010 cm−2 for E- and Z-1-cyano-1,3-butadiene, respectively. Our results are not consistent with those from Cooke et al. (2023, ApJ, 948, 133), who determine a column density of 3.8 × 1010 cm−2 for E-1-cyano-1,3-butadiene in TMC-1 using GBT data and a line stack technique. At the current level of sensitivity of our data, there is tentative evidence for the presence of the third cyano derivative isomer, 2-cyano-1,3-butadiene, although a firm detection must await more sensitive data. We derive an upper limit to its column density of 3.1 × 1010 cm−2. This isomer cannot be formed in the reaction between CN and 1,3-butadiene, according to experimental and theoretical studies, and thus we speculate whether it could arise from neutral-neutral reactions, such as C2 H3+CH2 CHCN and CH2 CCN+C2 H4. From the upper limit on the abundance of 1-cyano-1,3-butadiene derived here, we estimate that the abundance of 1,3-butadiene in TMC-1 is below 10−11−10−10 relative to H2. The low abundance inferred for 1,3-butadiene makes it unlikely that it plays an important role in bottom-up routes to cyclopentadiene and benzene.
Key words: astrochemistry / line: identification / ISM: molecules / radio lines: ISM / ISM: individual objects: TMC-1
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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