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Table 1

Host properties used to plot Fig. 1.

Spectral type M [ M ] R [ R ] r g

F0 1.6 1.44 0.25
F5 1.4 1.35 0.26
G5 0.92 0.81 0.38
K5 0.67 0.61 0.44
M0 0.51 0.45 0.50
M5 0.21 0.22 0.56

Notes. Spectral type and mass from Cox (2000), radius and gyration radius taken from CESAM stellar models (Morel 1997; Morel & Lebreton 2008) at the ZAMS.

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