Fig. 27
Pulsation periods of our set of low-mass He-core WD models in terms of the stellar mass, for radial (blue dashed lines), non-radial p-modes (blue solid lines) and g modes (red solid lines) at Teff, roughly the effective temperature measured for J111215.82+111745.0. Horizontal black segments (framed in a grey rectangle) represent the periods exhibited by this pulsating star.
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