Table 1: Main physical inputs of the stellar models for the various initial masses considered. The labels "r'' and "s'' indicate respectively the models computed with or without rotation while the labels A-D refer to the choices in nuclear reactions (see text and Table 2). The initial value of  $\Omega /\Omega _{\rm crit}$ is given. [I], [H02] and [H04] correspond respectively to Iliadis et al. (2001) and Hale et al. (2002,2004).
M ($M_\odot $) Label $\Omega /\Omega _{\rm crit}$ Nuclear rates
60 60rA 0.95 set A$^\dag $: NACRE (nominal)
  60rB 0.95 set B$^\dag $: [I, H02, H04] (nominal)
  60rC 0.95 set C$^\dag $: [I, H02, H04] (exp. limits)
  60rD 0.95 set D$^\dag $
  60rE 0.80 set C
20 20rC 0.95 set C
40 40rC 0.98 set C
120 120rC 0.80 set C
200 200rC 0.95 set C
20 20sC 0 set C
40 40sC 0 set C
60 40sC 0 set C
120 120sC 0 set C

$^\dag $ Details on the nuclear rates used are presented in Table 2.


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