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We employ two tabulated unified EOSs, FPS1 or SLy, at p > 5 x 1010 g cm 3. At lower densities, 108 g cm-3 < p < 5 x 1010 g cm-3, the crustal matter is described by the EOS of Haensel & Pichon (1994) (HP94), based on experimental nuclear data. This EOS is supplemented by the BPS EOS for cold catalyzed matter at p < 108 g cm-3(Chapter 3). The lowest-density parts of the tables at p < 105 g cm-3 have not been used in the fitting. At such low p the EOS is no longer one-parametric, but depends also on temperature (see Fig. 1.3).

1 The FPS table has been kindly provided by N. Stergioulas.

Table C.1. Parameters of the fit (C.2)

i

a¿ (FPS)

a¿(SLy)

i

a¿ (FPS)

a¿(SLy)

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