The Influence of Heavy Cosmic Rays in Energy Deposition in Molecular Clouds Employing the GEANT4 Code and Voyager I Data

2021 ◽  
Vol 921 (2) ◽  
pp. 116
Author(s):  
Sergio Pilling ◽  
Maurício Tizziani Pazianotto ◽  
Lucas Alves de Souza
2021 ◽  
Vol 911 (2) ◽  
pp. 129
Author(s):  
Mauricio Tizziani Pazianotto ◽  
Sergio Pilling ◽  
Jose Manuel Quesada Molina ◽  
Claudio Antonio Federico

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 ◽  
...  

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.


2021 ◽  
Vol 914 (2) ◽  
pp. 106
Author(s):  
A. Albert ◽  
R. Alfaro ◽  
C. Alvarez ◽  
J. R. Angeles Camacho ◽  
J. C. Arteaga-Velázquez ◽  
...  

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