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

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https://hal.archives-ouvertes.fr/hal-02867532
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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

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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⟩

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