Discovery of two cyano derivatives of acenaphthylene (C<sub>12</sub>H<sub>8</sub>) in TMC-1 with the QUIJOTE line survey

We report the discovery in TMC-1 of two cyano derivatives of the PAH acenaphthylene (C 12 H 8 ). We have found two series of lines with the QUIJOTE line survey that we assign to 1-C 12 H 7 CN and 5-C 12 H 7 CN. For the 1-isomer, we have detected and assigned 173 rotational transitions with J up to 46 and K a up to 9, corresponding to 107 independent frequencies. For the 5-isomer, the identification is based on 56 individual lines, corresponding to 117 rotational transitions with J up to 40 and K a up to 8. Identification of the carriers was achieved through a careful analysis of the derived rotational constants, which permit us to focus on molecules larger than naphthalene but smaller than anthracene and phenanthrene. Moreover, the derived rotational constants indicate that the species are planar; this allows us to discard derivatives of fluorene and acenaphthene, which are non-planar species. Quantum chemical calculations and subsequent chemical synthesis of these molecules, as well as the observation of their rotational transitions in the laboratory, unequivocally support our identifications. We also confirm, via a robust line-by-line detection, the previous claimed detection of 1- and 2-cyanonaphthalene, which were obtained through statistical stacking techniques. The column densities of 1- and 5-cyanoacenaphthylene are (9.5 ± 0.9) × 10 11 cm −2 , while those of 1- and 2-cyanonapthalene are (5.5 ± 0.5) × 10 11 cm −2 . Hence, it seems that acenaphthylene could be a factor of 1.7 more abundant than naphthalene. These results support a scenario in which PAHs grow in cold dark clouds based on fused five- and six-membered carbon rings.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-09-26
DOI
https://doi.org/10.1051/0004-6361/202452196
Citations
59
Primary Topic
Molecular Spectroscopy and Structure
Type
article
Field-Weighted Citation Impact
14.20

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article

Discovery of two cyano derivatives of acenaphthylene (C12H8) in TMC-1 with the QUIJOTE line survey

Alberto Lesarri, N. Marcelino, M. Agúndez, Jesús Janeiro et al.
59 citations
Astronomy and Astrophysics
Molecular Spectroscopy and Structure
14.20
article

Discovery of two cyano derivatives of acenaphthylene (C12H8) in TMC-1 with the QUIJOTE line survey

Alberto Lesarri, N. Marcelino, M. Agúndez, Jesús Janeiro, J. Cernicharo, C. Cabezas, Amanda L. Steber, Dolores Pérez, Yasuki Endo, R. Fuentetaja, Cristóbal Pérez, B. Tercero, Miguel Gullón Juanes, Ralf I. Kaiser, P. de Vicente
article en
59 citations

Abstract

We report the discovery in TMC-1 of two cyano derivatives of the PAH acenaphthylene (C 12 H 8 ). We have found two series of lines with the QUIJOTE line survey that we assign to 1-C 12 H 7 CN and 5-C 12 H 7 CN. For the 1-isomer, we have detected and assigned 173 rotational transitions with J up to 46 and K a up to 9, corresponding to 107 independent frequencies. For the 5-isomer, the identification is based on 56 individual lines, corresponding to 117 rotational transitions with J up to 40 and K a up to 8. Identification of the carriers was achieved through a careful analysis of the derived rotational constants, which permit us to focus on molecules larger than naphthalene but smaller than anthracene and phenanthrene. Moreover, the derived rotational constants indicate that the species are planar; this allows us to discard derivatives of fluorene and acenaphthene, which are non-planar species. Quantum chemical calculations and subsequent chemical synthesis of these molecules, as well as the observation of their rotational transitions in the laboratory, unequivocally support our identifications. We also confirm, via a robust line-by-line detection, the previous claimed detection of 1- and 2-cyanonaphthalene, which were obtained through statistical stacking techniques. The column densities of 1- and 5-cyanoacenaphthylene are (9.5 ± 0.9) × 10 11 cm −2 , while those of 1- and 2-cyanonapthalene are (5.5 ± 0.5) × 10 11 cm −2 . Hence, it seems that acenaphthylene could be a factor of 1.7 more abundant than naphthalene. These results support a scenario in which PAHs grow in cold dark clouds based on fused five- and six-membered carbon rings.

Astronomy and AstrophysicsVol. 690
Universidad de Valladolid (ES), University of Hawaiʻi at Mānoa (US), National Yang Ming Chiao Tung University (TW), Universidade de Santiago de Compostela (ES), Instituto de Física Fundamental (ES), Center for Research in Molecular Medicine and Chronic Diseases (ES), Yebes Observatory (ES), Spanish National Observatory (ES)
European Commission, Ministry of Science and Technology, Taiwan, Ministerio de Ciencia e Innovación, Xunta de Galicia, European Research Council, Consejo Superior de Investigaciones Científicas, European Regional Development Fund, Agencia Estatal de Investigación
Openalex Percentile: Top 0%
Molecular Spectroscopy and Structure
14.20
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