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pro vyhledávání: '"Gavardi, E."'
H2 formation is an important process in post-shock regions, since H2 is an active participant in the cooling and shielding of the environment. The onset of H2 formation therefore has a strong effect on the temperature and chemical evolution in the po
Externí odkaz:
http://arxiv.org/abs/1005.1847
The formation of H2 in the interstellar medium proceeds on the surfaces of silicate or carbonaceous particles. To get a deeper insight of its formation on the latter substrate, this letter focuses on H2 desorption from graphite (0001) in Temperature-
Externí odkaz:
http://arxiv.org/abs/0907.3361
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters; Jul2010, Vol. 406 Issue 1, pL11-L15, 5p, 1 Chart, 3 Graphs
