Fig. 20

Upper panel: the relation between
σPθ and
MG for supergiants and bright giants,
assuming either an exponential (red plusses) or a parabola (blue crosses) to connect
the box-in-a-star with the star-in-a-box models (Fig. 18). The equation of the dashed green line (through the red plusses) is
, whereas
the equation of the magenta dotted line (through the blue crosses) is
.
Lower panel: same as the upper panel, for the relation between
the pressure scale height Hp and the absolute magnitude in the Gaia
G band. Only stars with a detectable photocentric motion (for the
exponential fit: red crosses; for the parabolic fit: green dot) have been plotted.
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