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Matteo Cantiello edited MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex
almost 9 years ago
Commit id: 96b93060fc0ebc895d477c8b6993d447451a554b
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diff --git a/MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex b/MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex
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giants that do not burn helium in their cores \citep{Stello_2013,Mosser_2014}.
It is striking how the stars form two distinct branches that gradually merge as the stars
evolve towards lower \numax. % This trend is also evident in Fig.1.
Most stars fall on the
``normal" ``normal'' upper branch of visibilities around 1.5 in
agreement with previous results \citep{Mosser_2011}.
The agreement with the theoretically predicted location of the
suppressed branch (black curve) is remarkable. This curve assumes that all the wave energy leaking into the stellar core is trapped; the decrease of the suppression towards lower \numax\ is a consequence of the increasingly weaker coupling between acoustic waves in the envelope and gravity waves in the core as stars evolve (Fuller et al. 2015).