Pulsations in M dwarf stars

Preprint English OPEN
Rodríguez-López, C.; MacDonald, J.; Moya, A.;
(2011)

We present the results of the first theoretical non-radial non-adiabatic pulsational study of M dwarf stellar models with masses in the range 0.1 to 0.5M_solar. We find the fundamental radial mode to be unstable due to an \epsilon mechanism caused by deuterium (D-) burn... View more
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