Evolution of Fluorine in the Galaxy with the ν-process
We calculate the evolution of fluorine in the solar neighborhood with the ν-process of core-collapse supernovae, the results of which are in good agreement with the observations of field stars. The ν-process operating in supernovae causes the [F/O] rati
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Kobayashi_Evolution_of_Fluorine_in_the_2011.pdf||172.79 kB||Adobe PDF|
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