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Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration

[Image: see text] Gas phase electronic spectra of pure carbon cations generated by laser vaporization of graphite in a supersonic jet and cooled to below 10 K and tagged with helium atoms in a cryogenic trap are presented. The measured C(2n)(+)–He with n from 6 to 14, are believed to be monocyclic r...

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Autores principales: Rademacher, Johanna, Reedy, Elliott S., Campbell, Ewen K.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Chemical Society 2022
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9007455/
https://www.ncbi.nlm.nih.gov/pubmed/35344354
http://dx.doi.org/10.1021/acs.jpca.2c00650
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author Rademacher, Johanna
Reedy, Elliott S.
Campbell, Ewen K.
author_facet Rademacher, Johanna
Reedy, Elliott S.
Campbell, Ewen K.
author_sort Rademacher, Johanna
collection PubMed
description [Image: see text] Gas phase electronic spectra of pure carbon cations generated by laser vaporization of graphite in a supersonic jet and cooled to below 10 K and tagged with helium atoms in a cryogenic trap are presented. The measured C(2n)(+)–He with n from 6 to 14, are believed to be monocyclic ring structures and possess an origin band wavelength that shifts linearly with the number of carbon atoms, as recently demonstrated through N(2) tagging by Buntine et al. (J. Chem. Phys.2021, 155, 21430234879679). The set of data presented here further constrains the spectral characteristics inferred for the bare C(2n)(+) ions to facilitate astronomical searches for them in diffuse clouds by absorption spectroscopy.
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spelling pubmed-90074552022-04-14 Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration Rademacher, Johanna Reedy, Elliott S. Campbell, Ewen K. J Phys Chem A [Image: see text] Gas phase electronic spectra of pure carbon cations generated by laser vaporization of graphite in a supersonic jet and cooled to below 10 K and tagged with helium atoms in a cryogenic trap are presented. The measured C(2n)(+)–He with n from 6 to 14, are believed to be monocyclic ring structures and possess an origin band wavelength that shifts linearly with the number of carbon atoms, as recently demonstrated through N(2) tagging by Buntine et al. (J. Chem. Phys.2021, 155, 21430234879679). The set of data presented here further constrains the spectral characteristics inferred for the bare C(2n)(+) ions to facilitate astronomical searches for them in diffuse clouds by absorption spectroscopy. American Chemical Society 2022-03-28 2022-04-07 /pmc/articles/PMC9007455/ /pubmed/35344354 http://dx.doi.org/10.1021/acs.jpca.2c00650 Text en © 2022 American Chemical Society https://creativecommons.org/licenses/by/4.0/Permits the broadest form of re-use including for commercial purposes, provided that author attribution and integrity are maintained (https://creativecommons.org/licenses/by/4.0/).
spellingShingle Rademacher, Johanna
Reedy, Elliott S.
Campbell, Ewen K.
Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration
title Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration
title_full Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration
title_fullStr Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration
title_full_unstemmed Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration
title_short Electronic Spectroscopy of Monocyclic Carbon Ring Cations for Astrochemical Consideration
title_sort electronic spectroscopy of monocyclic carbon ring cations for astrochemical consideration
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9007455/
https://www.ncbi.nlm.nih.gov/pubmed/35344354
http://dx.doi.org/10.1021/acs.jpca.2c00650
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