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

Gavilan, L. ; Lemaire, J. ; Vidali, G.

Monthly notices of the Royal Astronomical Society, 2012-08, Vol.424 (4), p.2961-2970 [Periódico revisado por pares]

Oxford University Press (OUP): Policy P - Oxford Open Option A

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Laboratory evidence for the non-detection of excited nascent H2 in dark clouds
Laboratory evidence for the non-detection of excited nascent H2 in dark clouds
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Laboratory evidence for the non-detection of excited nascent H2 in dark clouds

Congiu, E. ; Matar, E. ; Kristensen, L. E. ; Dulieu, F. ; Lemaire, J. L.

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.397 (1), p.L96-L100 [Periódico revisado por pares]

Oxford, UK: Blackwell Publishing Ltd

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Morphology of the solid water synthesized through the pathway D + O2 studied by the sensitive TPD technique
Morphology of the solid water synthesized through the pathway D + O2 studied by the sensitive TPD technique
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Morphology of the solid water synthesized through the pathway D + O2 studied by the sensitive TPD technique

Accolla, M ; Congiu, E ; Manicò, G ; Dulieu, F ; Chaabouni, H ; Lemaire, J. L ; Pirronello, V

Monthly notices of the Royal Astronomical Society, 2013-03, Vol.429 (4), p.3200-3206 [Periódico revisado por pares]

Oxford University Press

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