Jim Fuller edited section_Segue_to_RGs_maybe__.tex  almost 9 years ago

Commit id: a616437a70f671de5207b620c842f8acea578db9

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%[REF Bedding2011/Stello2013/Mosser2014]   and to measure radial differential rotation \citep{Beck_2011,Mosser_2012}.   This fortune arises because %[through resonance coupling where]  each acoustic non-radial envelope mode couple couples  to multiple gravity modes in the core core,  forming several observable  mixed modes %observable at the surface, with frequenciesobservable  in the vicinity of the acoustic mode \citep{Beck_2011}. This coupling is strongest for dipole modes making them the most useful  probes of the core \citep{Dupret_2009}. %[REF Unno/Dupret?].