H-2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations

Wakelam, Valentine; Bron, Emeric; Cazaux, Stephanie; Dulieu, Francois; Gry, Cecile; Guillard, Pierre; Habart, Emilie; Hornekaer, Liv; Morisset, Sabine; Nyman, Gunnar; Pirronello, Valerio; Price, Stephen D.; Valdivia, Valeska; Vidali, Gianfranco; Watanabe, Naoki

doi:10.1016/j.molap.2017.11.001

Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form and survive photo-dissociation in tenuous environments. Its formation involves catalytic reactions on the surface of interstellar grains. The micro-physics of the formation process has been investigated intensively in the last 20 years, in parallel of new astrophysical observational and modeling progresses. In the perspectives of the probable revolution brought by the future satellite JWST, this article has been written to present what we think we know about the H-2 formation in a variety of interstellar environments

Titolo:	H-2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations
Autori interni:	Wakelam, Valentine Bron, Emeric Cazaux, Stephanie Dulieu, Francois Gry, Cecile Guillard, Pierre Habart, Emilie Hornekaer, Liv Morisset, Sabine Nyman, Gunnar PIRRONELLO, Valerio Price, Stephen D. Valdivia, Valeska Vidali, Gianfranco Watanabe, Naoki mostra contributor esterni nascondi contributor esterni
Data di pubblicazione:	2017
Rivista:	MOLECULAR ASTROPHYSICS
Handle:	http://hdl.handle.net/20.500.11769/334033
Appare nelle tipologie:	1.1 Articolo in rivista

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http://hdl.handle.net/20.500.11769/334033

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