Polycyclic Aromatic Hydrocarbons (PAHs) in Interstellar Ices: A Computational Study into How the Ice Matrix Influences the Ionic State of PAH Photoproducts-Reference-Cited by-同舟云学术

Polycyclic Aromatic Hydrocarbons (PAHs) in Interstellar Ices: A Computational Study into How the Ice Matrix Influences the Ionic State of PAH Photoproducts

Published:2022-02-21 Issue:3 Volume:6 Page:766-774
ISSN:2472-3452
Container-title:ACS Earth and Space Chemistry
language:en
Short-container-title:ACS Earth Space Chem.

Author:

ten Brinck Stephanie¹,Nieuwland Celine¹^ORCID,van der Werf Angela¹,Veenboer Richard M. P.¹^ORCID,Linnartz Harold²^ORCID,Bickelhaupt F. Matthias¹³^ORCID,Fonseca Guerra Célia¹⁴^ORCID

Affiliation:

1. Department of Theoretical Chemistry, Amsterdam Institute of Molecular and Life Sciences (AIMMS), Amsterdam Center for Multiscale Modeling (ACMM), Vrije Universiteit Amsterdam, De Boelelaan 1083, 1081 HV Amsterdam, The Netherlands

2. Laboratory for Astrophysics, Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands

3. Institute for Molecules and Materials (IMM), Radboud University, Heyendaalseweg 135, 6525 AJ Nijmegen, The Netherlands

4. Leiden Institute of Chemistry, Gorlaeus Laboratories, Leiden University, Einsteinweg 55, 2333 CC Leiden, The Netherlands

Funder

Nederlandse Organisatie voor Wetenschappelijk Onderzoek

Publisher

American Chemical Society (ACS)

Subject

Space and Planetary Science,Atmospheric Science,Geochemistry and Petrology

Link

https://pubs.acs.org/doi/pdf/10.1021/acsearthspacechem.1c00433

Reference54 articles.

1. 8-13 micron spectra of NGC 7027, BD +30 3639 and NGC 6572.

2. Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands - Auto exhaust along the Milky Way

3. Interstellar polycyclic aromatic hydrocarbons - The infrared emission bands, the excitation/emission mechanism, and the astrophysical implications

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