| Issue |
A&A
Volume 705, January 2026
|
|
|---|---|---|
| Article Number | L7 | |
| Number of page(s) | 8 | |
| Section | Letters to the Editor | |
| DOI | https://doi.org/10.1051/0004-6361/202557893 | |
| Published online | 07 January 2026 | |
Letter to the Editor
Discovery of two new isomers of cyanoacenaphthylene (C12H7CN) in the Taurus molecular cloud 1 with the QUIJOTE line survey
1
Dept. de Astrofísica Molecular, Instituto de Física Fundamental (IFF-CSIC), C/ Serrano 121, 28006 Madrid, Spain
2
Centro de Desarrollos Tecnológicos, Observatorio de Yebes (IGN), 19141 Yebes, Guadalajara, Spain
3
Observatorio Astronómico Nacional (OAN, IGN), C/ Alfonso XII, 3, 28014 Madrid, Spain
4
Centro Singular de Investigación en Química Biolóxica e Materiais Moleculares (CiQUS) and Departamento de Química Orgánica, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain
5
Departamento de Química Física y Química Inorgánica, Facultad de Ciencias-I.U. CINQUIMA, Universidad de Valladolid, 47011 Valladolid, Spain
⋆ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
29
October
2025
Accepted:
19
November
2025
We report the discovery of the 3- and 4-cyano isomers of acenaphthylene (C12H8) using the QUIJOTE line survey of the Taurus molecular cloud 1 (TMC-1). The frequency range of the line survey in the Q band (31.2–50.3 GHz) was complemented with data from a new receiver installed at the Yebes 40m radio telescope that covers the K and Ka bands (18–32 GHz). The identification of 3-cyanoacenaphthylene was based on the detection of 135 individual lines that correspond to 194 rotational transitions. For 4-cyanoacenaphthylene, the lines are slightly weaker, but we identified 37 individual lines that correspond to 66 rotational transitions. As a first step for the identification, we compared the derived rotational constants with their expected theoretical values and obtained a match better than 0.2%. Finally, the new isomers were synthesized in our chemical laboratory and observed in our microwave spectroscopic facilities. The derived laboratory constants match those derived from TMC-1 data perfectly, which confirms our identifications. Lines in the K − Ka band from the previously detected isomers 1- and 5-cyanoacenaphthylene are also reported. The derived column density for 3-cyanoacenaphthylene is (7.0 ± 0.7) × 1011 cm−2, and for the 4-cyano isomer, we derive a column density of (5.0 ± 0.6) × 1011 cm−2. The four possible isomers of cyanoacenaphthylene are finally found in TMC-1. Despite their high relative energies, they exhibit similar abundances (within a factor of ∼2).
Key words: astrochemistry / line: identification / molecular data / ISM: general / ISM: molecules / ISM: individual objects: TMC-1
© The Authors 2026
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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