deletions | additions       diff --git a/section_Segue_to_RGs_maybe__.tex b/section_Segue_to_RGs_maybe__.tex  index 667d0ef..defe71d 100644  --- a/section_Segue_to_RGs_maybe__.tex  +++ b/section_Segue_to_RGs_maybe__.tex 
...
%stars evolve]  Both low- % solar-like   and intermediate-mass stars evolve to become  red giants when their hydrogen core hydrogen-core  burning is exhausted. Like the Sun, red giants, show a broad comb-like frequency spectrum of radial and non-radial  acoustic oscillation modes excited by turbulent surface convection \citep{De_Ridder_2009}.  The observed mode power across the spectrum has an overall bell-like