Role of Ga2O in the removal of GaAs surface oxides induced by atomic hydrogen

1994 ◽  
Vol 12 (4) ◽  
pp. 1858-1863 ◽  
Author(s):  
Yuichi Ide ◽  
Masamichi Yamada
Keyword(s):  
Atomic Hydrogen ◽  
Gaas Surface ◽  
Surface Oxides

Role of atomic hydrogen diffusion in a hydrogen flame

2007 ◽  
Vol 43 (2) ◽  
pp. 125-131 ◽  
Author(s):  
V. A. Bunev ◽  
V. N. Panfilov ◽  
V. S. Babkin
Keyword(s):  
Atomic Hydrogen ◽  
Hydrogen Diffusion ◽  
Hydrogen Flame

A novel assessment of the role of the methyl radical and water formation channel in the CH3OH + H reaction

2017 ◽  
Vol 19 (36) ◽  
pp. 24467-24477 ◽  
Author(s):  
Flávio O. Sanches-Neto ◽  
Nayara D. Coutinho ◽  
Valter H. Carvalho-Silva
Keyword(s):  
Atomic Hydrogen ◽  
Methyl Radical ◽  
Water Formation

A number of experimental and theoretical papers accounted almost exclusively for two channels in the reaction of atomic hydrogen with methanol. However, several astrochemical studies claimed the importance of another channel for this reaction.

scholarly journals The atomic hydrogen/molecular cloud association: an unavoidable relationship

1991 ◽  
Vol 147 ◽  
pp. 37-40
Author(s):  
G. Joncas
Keyword(s):  
Atomic Hydrogen ◽  
Molecular Clouds ◽  
Large Scale ◽  
Young Stars ◽  
Physical Processes ◽  
Star Forming ◽  
Dark Clouds ◽  
Star Forming Regions ◽  
The Impact

The presence of HI in the interstellar medium is ubiquitous. HI is the principal actor in the majority of the physical processes at work in our Galaxy. Restricting ourselves to the topics of this symposium, atomic hydrogen is involved with the formation of molecular clouds and is one of the byproducts of their destruction by young stars. HI has different roles during a molecular cloud's life. I will discuss here a case of coexisting HI and H2 at large scale and the origin of HI in star forming regions. For completeness' sake, it should be mentionned that there are at least three other aspects of HI involvement: HI envelopes around molecular clouds, the impact of SNRs (see work on IC 443), and the role of HI in quiescent dark clouds (see van der Werf's work).

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