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Published in 2019 at "Frontiers in Astronomy and Space Sciences"
DOI: 10.3389/fspas.2019.00076
Abstract: Recent fully non-adiabatic theoretical studies of M dwarf models show that they have the potential to excite radial\textbf{,} and low-order, low-degree non-radial modes, as well as solar-like oscillations, due to models being completely convective or…
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Keywords:
quest pulsating;
pulsating dwarf;
dwarf stars;
spectroscopy ... See more keywords