deletions | additions       diff --git a/Our_results_show_that_main__.tex b/Our_results_show_that_main__.tex  index e921d61..3e77b19 100644  --- a/Our_results_show_that_main__.tex  +++ b/Our_results_show_that_main__.tex 
...
momentum to help explain the measured rotation rates of red giant cores  \citep{Mosser_2012,Cantiello_2014}.   {\bf The presence of strong internal magnetic fields might help explain the extra internal mixing observed in   red giant and asymptotic giant stars \citep{Busso_2007}. Interestingly theamplitude of  magnetic fields field strength  necessary forthe  magnetic buoyancy mixing \citep{Nucci_2014} is similar to the fields amplitude field strength  required for dipole modes mode  suppression \citep{Fuller15}.}    
...