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Glitches in solar-like oscillating F-type stars: Possible contribution of non-linear terms

Glitches in solar-like oscillating F-type stars: Possible contribution of non-linear terms

The glitch signatures in $r_{010}$ for F-type stars (higher amplitude and period of the oscillatory component) are very different from those of G-type stars. The aim of this work is to analyse the signatures of these glitches and understand the origin of the differences in these signatures between G-type and …