scholarly journals Grain-surface reactions in molecular clouds: the effect of cosmic rays and quantum tunnelling

2014 ◽  
Vol 440 (4) ◽  
pp. 3557-3567 ◽  
Author(s):  
L. Reboussin ◽  
V. Wakelam ◽  
S. Guilloteau ◽  
F. Hersant
2002 ◽  
Vol 12 ◽  
pp. 55-57 ◽  
Author(s):  
Eric Herbst

AbstractIt is impossible to explain the abundances of some gas-phase and most condensed-phase interstellar molecules without the use of grain chemistry. Nevertheless, grain-surface chemistry is relatively poorly understood for a variety of reasons. Our current knowledge of this chemistry and its use in interstellar models is discussed along with specific needs for future research.


2015 ◽  
Vol 805 (1) ◽  
pp. 50 ◽  
Author(s):  
Ryan D. Abrahams ◽  
Timothy A. D. Paglione

2008 ◽  
Author(s):  
Stefano Gabici ◽  
Sabrina Casanova ◽  
Felix A. Aharonian ◽  
Felix A. Aharonian ◽  
Werner Hofmann ◽  
...  

1976 ◽  
Vol 44 (2) ◽  
pp. 385-388 ◽  
Author(s):  
M. A. Leitch-Devlin ◽  
T. J. Millar ◽  
J. Pickles ◽  
D. A. Williams

1982 ◽  
Vol 259 ◽  
pp. 859 ◽  
Author(s):  
E. G. Zweibel ◽  
J. M. Shull
Keyword(s):  

1981 ◽  
Vol 94 ◽  
pp. 309-319 ◽  
Author(s):  
A. W. Wolfendale

It is shown that there is evidence favouring molecular clouds being sources of γ-rays, the fluxes being consistent with expectation for ambient cosmic rays interacting with the gas in the clouds for the clouds considered. An estimate is made of the fraction of the apparently diffuse γ-ray flux which comes from cosmic ray interactions in the I.S.M. as distinct from unresolved discrete sources. Finally, an examination is made of the possibility of gradients of cosmic ray intensity in the Galaxy.


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