Efficiency of molecular hydrogen formation on silicates

被引:161
|
作者
Pirronello, V
Biham, O
Liu, C
Shen, LO
Vidali, G
机构
[1] SYRACUSE UNIV, SOLID STATE SCI & TECHNOL PROGRAM, SYRACUSE, NY 13244 USA
[2] SYRACUSE UNIV, DEPT PHYS, SYRACUSE, NY 13244 USA
[3] CATANIA UNIV, IST FIS, CATANIA, SICILY, ITALY
[4] HEBREW UNIV JERUSALEM, RACAH INST PHYS, IL-91904 JERUSALEM, ISRAEL
关键词
dust; extinction; ISM; abundances; molecules; molecular processes;
D O I
10.1086/310746
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on laboratory measurements of molecular hydrogen formation and recombination on an olivine slab as a function of surface temperature under conditions relevant to those encountered in the interstellar medium. On the basis of our experimental evidence, we recognize that there are two main regimes of H coverage that are of astrophysical importance; for each of them we provide an expression giving the production rate of molecular hydrogen in interstellar clouds.
引用
收藏
页码:L131 / L134
页数:4
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