H 2 Formation on Interstellar Dust Grains: The Viewpoints of Theory, Experiments, Models and Observations

Stephanie Cazaux*

*Corresponding author for this work

Research output: Chapter in Book/Conference proceedings/Edited volumeConference contributionScientificpeer-review

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Abstract

Molecular hydrogen (H 2 ) is the most abundant molecule in the Universe. Its formation involves catalytic reactions occurring on the surface of interstellar dust grains, but also involving polycyclic aromatic hydrocarbons (PAHs). Experiments and theoretical calculations have been performed to determine the processes governing the formation of H 2 on dust and involving PAHs. These studies were recently brought in a review paper (Wakelam et al. 2017), from which this contribution is based.

Original languageEnglish
Title of host publicationEuropean Conference on Laboratory Astrophysics ECLA2020 - The Interplay of Dust, Ice, and Gas in Space
EditorsVito Mennella, Christine Joblin
PublisherSpringer
Pages151-159
Number of pages9
ISBN (Print)9783031290022
DOIs
Publication statusPublished - 2023
EventEuropean Conference on Laboratory Astrophysics, ECLA 2020 - Anacapri, Italy
Duration: 26 Sept 20211 Oct 2021

Publication series

NameAstrophysics and Space Science Proceedings
Volume59
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605

Conference

ConferenceEuropean Conference on Laboratory Astrophysics, ECLA 2020
Country/TerritoryItaly
CityAnacapri
Period26/09/211/10/21

Bibliographical note

Green Open Access added to TU Delft Institutional Repository ‘You share, we take care!’ – Taverne project https://www.openaccess.nl/en/you-share-we-take-care
Otherwise as indicated in the copyright section: the publisher is the copyright holder of this work and the author uses the Dutch legislation to make this work public.

Keywords

  • ISM
  • Molecular hydrogen
  • Molecules

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