deletions | additions       diff --git a/abstract.tex b/abstract.tex  index 9124b88..9c5d069 100644  --- a/abstract.tex  +++ b/abstract.tex 
...
formation process \citep{2008CoSka..38..443P}. These stars do have convective cores that might produce  internal magnetic fields \citep{Brun_2005}, and these might even survive into later stages of stellar  evolution, but information is limited by our inability to measure the  fields below the stellar surface. surface \citep{Auri_re_2015}.  Here we use asteroseismology to study the occurrence of magnetic fields in the cores of low- and  intermediate-mass stars. We have measured the strength of dipolar  oscillation modes, which are suppressed by a strong magnetic field in the