H2, HD, and D2abundances on ice-covered dust grains in dark clouds

Author:

Kristensen L. E.,Amiaud L.,Fillion J.-H.,Dulieu F.,Lemaire J.-L.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. Amiaud, L. 2006, Ph.D. Thesis, Université de Cergy-Pontoise, http://tel.archives-ouvertes.fr/tel-00124797/en/

2. Interaction of D2 with H2O amorphous ice studied by temperature-programed desorption experiments

3. Interaction of atomic and molecular deuterium with a nonporous amorphous water ice surface between 8 and 30K

4. Measurement of the Adsorption Energy Difference betweenOrtho- andPara-D2on an Amorphous Ice Surface

5. Ballesteros-Paredes, J., Klessen, R. S., Mac Low, M.-M., & Vazquez-Semadeni, E. 2007, in Protostars and Planets V, ed. B. Reipurth, D. Jewitt, & K. Keil, 63

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2. Experimental H2O formation on carbonaceous dust grains at temperatures up to 85 K;Monthly Notices of the Royal Astronomical Society;2023-12-18

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