On the Mechanism of H2 Formation in the Interstellar Medium

1987 ◽  
pp. 167-169
Author(s):  
Valerio Pirronello
1987 ◽  
Vol 120 ◽  
pp. 167-169
Author(s):  
Valerio Pirronello

The problem of the formation of molecular hydrogen in interstellar clouds is revisited. the role played by cosmic ray bombardment under certain circumstances is considered mainly in the light of the low formation rate of H2 on grains due to the reduced mobility of adsorbed H atoms on their amorphous surfaces at interstellar temperatures.


2012 ◽  
Vol 421 (3) ◽  
pp. 2531-2542 ◽  
Author(s):  
Milica Micic ◽  
Simon C. O. Glover ◽  
Christoph Federrath ◽  
Ralf S. Klessen

Author(s):  
M. G. Medvedev ◽  
◽  
A. B. Ostrovskii ◽  
A. I. Vasyunin ◽  
◽  
...  

We realized stochastic model evaluating efficency of recombination H2 in interstellar medium based on the approach of the continious-time random walk on two-dimentional lattice. This method allows to model inhomogeneous surfaces. We estimate recombination efficiensy as a function of model parameters. The influence of uncertainty of diffusion/desorption energy ratio on molecular hydrogen recombination was considered also.


2002 ◽  
Vol 391 (2) ◽  
pp. 675-680 ◽  
Author(s):  
C. Gry ◽  
F. Boulanger ◽  
C. Nehmé ◽  
G. Pineau des Forêts ◽  
E. Habart ◽  
...  

2002 ◽  
Vol 4 ◽  
pp. 9-9
Author(s):  
I. Ristorcelli ◽  
B. Stepnik ◽  
X. Dupac ◽  
A. Abergel ◽  
J. P. Bernard ◽  
...  

2018 ◽  
Author(s):  
Emmanuel E. Etim ◽  
Prasanta Gorai ◽  
Ankan Das ◽  
Sandip K. Chakrabarti ◽  
Elangannan Arunan

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