HAL will be down for maintenance from Friday, June 10 at 4pm through Monday, June 13 at 9am. More information
Skip to Main content Skip to Navigation
Journal articles

Are molecule-covered dust grains efficient catalysts of H2 formation in the cold ISM?

L. Gavilan 1 J. Lemaire 2, 1 G. Vidali 1
1 LERMA - Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique
2 LRGP - Laboratoire Réactions et Génie des Procédés
Document type :
Journal articles
Complete list of metadata
https://hal.archives-ouvertes.fr/hal-02867532
Contributor : La. Bibliotheque Connect in order to contact the contributor
Submitted on : Friday, January 28, 2022 - 6:31:00 AM
Last modification on : Thursday, March 17, 2022 - 10:08:23 AM
Long-term archiving on: : Friday, April 29, 2022 - 6:11:04 PM

File

Vignette du document
424-4-2961.pdf
Publisher files allowed on an open archive

Licence

Distributed under a Creative Commons Attribution 4.0 International License

Identifiers

Collections

OBSPM | SU-TI | SU-SCIENCES | SORBONNE-UNIVERSITE | PSL | LRGP-UL | UNIV-LORRAINE | LERMA | UNIV-CERGY | CNRS | UPMC | ENS-PARIS | INSU

Citation

L. Gavilan, J. Lemaire, G. Vidali. Are molecule-covered dust grains efficient catalysts of H2 formation in the cold ISM?. Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2012, 424 (4), pp.2961-2970. ⟨10.1111/j.1365-2966.2012.21463.x⟩. ⟨hal-02867532⟩

Export

BibTeX TEI DC DCterms EndNote Datacite

Share

Metrics

Record views

45

Files downloads

3