deletions | additions       diff --git a/figures/b_crit_nu_mass1/caption.tex b/figures/b_crit_nu_mass1/caption.tex  index 30f1115..8ba8d70 100644  --- a/figures/b_crit_nu_mass1/caption.tex  +++ b/figures/b_crit_nu_mass1/caption.tex 
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inferred asteroseismic mass. The coloured contours indicate the minimum  radial component of the magnetic field at the hydrogen shell required for  mode suppression (the critical field, $B_c$). Filled red  circles markthe  stars with observed suppressed modes, and open circles mark normal (not suppressed) stars. The cross shows a typical errorbar for the data points.   The uncertainty in $B_c$ due to uncertainty in mass is negligible for stars below 1.4\msol\ and is no  more than 25\% for the more massive stars.