Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds

The abundances of small Polycyclic Aromatic Hydrocarbons (PAHs) observed in interstellar clouds has surprised astronomers and confounded astrochemical models. Here, the authors show that fast radiative cooling by Recurrent Fluorescence efficiently stabilizes the small PAH cation 1-cyanonaphthalene.

Bibliographic Details
Main Authors: Mark H. Stockett, James N. Bull, Henrik Cederquist, Suvasthika Indrajith, MingChao Ji, José E. Navarro Navarrete, Henning T. Schmidt, Henning Zettergren, Boxing Zhu
Format: Article
Language:English
Published: Nature Portfolio 2023-01-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-023-36092-0
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author Mark H. Stockett
James N. Bull
Henrik Cederquist
Suvasthika Indrajith
MingChao Ji
José E. Navarro Navarrete
Henning T. Schmidt
Henning Zettergren
Boxing Zhu
author_facet Mark H. Stockett
James N. Bull
Henrik Cederquist
Suvasthika Indrajith
MingChao Ji
José E. Navarro Navarrete
Henning T. Schmidt
Henning Zettergren
Boxing Zhu
author_sort Mark H. Stockett
collection DOAJ
description The abundances of small Polycyclic Aromatic Hydrocarbons (PAHs) observed in interstellar clouds has surprised astronomers and confounded astrochemical models. Here, the authors show that fast radiative cooling by Recurrent Fluorescence efficiently stabilizes the small PAH cation 1-cyanonaphthalene.
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spelling doaj.art-76a69a384a9043afa1fbe1f6842b31f22023-01-29T12:17:24ZengNature PortfolioNature Communications2041-17232023-01-011411810.1038/s41467-023-36092-0Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar cloudsMark H. Stockett0James N. Bull1Henrik Cederquist2Suvasthika Indrajith3MingChao Ji4José E. Navarro Navarrete5Henning T. Schmidt6Henning Zettergren7Boxing Zhu8Department of Physics, Stockholm UniversitySchool of Chemistry, University of East AngliaDepartment of Physics, Stockholm UniversityDepartment of Physics, Stockholm UniversityDepartment of Physics, Stockholm UniversityDepartment of Physics, Stockholm UniversityDepartment of Physics, Stockholm UniversityDepartment of Physics, Stockholm UniversityDepartment of Physics, Stockholm UniversityThe abundances of small Polycyclic Aromatic Hydrocarbons (PAHs) observed in interstellar clouds has surprised astronomers and confounded astrochemical models. Here, the authors show that fast radiative cooling by Recurrent Fluorescence efficiently stabilizes the small PAH cation 1-cyanonaphthalene.https://doi.org/10.1038/s41467-023-36092-0
spellingShingle Mark H. Stockett
James N. Bull
Henrik Cederquist
Suvasthika Indrajith
MingChao Ji
José E. Navarro Navarrete
Henning T. Schmidt
Henning Zettergren
Boxing Zhu
Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds
Nature Communications
title Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds
title_full Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds
title_fullStr Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds
title_full_unstemmed Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds
title_short Efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small PAHs in interstellar clouds
title_sort efficient stabilization of cyanonaphthalene by fast radiative cooling and implications for the resilience of small pahs in interstellar clouds
url https://doi.org/10.1038/s41467-023-36092-0
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