Fig. 3
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Adiabats obtained from different EOSs and corresponding to a homogeneous model, with no compact core, with Y = 0.245. Table 1 lists the details of the EOSs. Below are shown the contribution functions of the gravitational moments of order 0 to 8 centred at their peak. Their extent corresponds to their full width at half maximum (see Guillot 2005 for more details).
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