[HTML][HTML] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, S Baouche, F Dulieu, E Matar… - Astronomy & …, 2012 - aanda.org
Context. Sticking of H and D atoms on interstellar dust grains is the first step in molecular
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions.
H Chaabouni, H Bergeron, S Baouche… - Astronomy & …, 2012 - search.ebscohost.com
Context. Sticking of H and D atoms on interstellar dust grains is the first step in molecular
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche… - Astronomy and …, 2012 - ui.adsabs.harvard.edu
Context. Sticking of H and D atoms on interstellar dust grains is the first step in molecular
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
[引用][C] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H CHAABOUNI, H BERGERON… - Astronomy and …, 2012 - pascal-francis.inist.fr
Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
CNRS Inist Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple …
CNRS Inist Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple …
[PDF][PDF] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche, F Dulieu… - A&A, 2012 - scholar.archive.org
Context. Sticking of H and D atoms on interstellar dust grains is the first step in molecular
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche, F Dulieu… - arXiv preprint arXiv …, 2012 - arxiv.org
Sticking of H and D atoms on interstellar dust grains is the first step in molecular hydrogen
formation, which is a key reaction in the InterStellar Medium (ISM). After studying the sticking …
formation, which is a key reaction in the InterStellar Medium (ISM). After studying the sticking …
[PDF][PDF] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche, F Dulieu… - A&A, 2012 - researchgate.net
Context. Sticking of H and D atoms on interstellar dust grains is the first step in molecular
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
[PDF][PDF] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche, F Dulieu… - A&A, 2012 - lassie.u-cergy.fr
Context. Sticking of H and D atoms on interstellar dust grains is the first step in molecular
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
hydrogen formation, which is a key reaction in the interstellar medium. Isotopic properties of …
[引用][C] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche… - Astronomy and …, 2012 - inria.hal.science
Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions - Inria -
Institut national de recherche en sciences et technologies du numérique Accéder directement …
Institut national de recherche en sciences et technologies du numérique Accéder directement …
[引用][C] Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
H Chaabouni, H Bergeron, S Baouche… - Astronomy & …, 2012 - cir.nii.ac.jp