All Tables

Table 1: Total crustal heating $Q_{\rm tot}$ for $A_{\rm i}=56$ and $A_{\rm i}=106$ .
Table A.1: Non-equilibrium processes in the crust of an accreting neutron stars assuming that the X-ray ashes consist of pure $^{106}{\rm Pd}$ .
Table A.2: Nuclear processes and released heat in the inner crust, assuming initial ashes of pure $^{106}{\rm Pd}$ (i.e. as in Table A.1) but suppressing pycnonuclear fusion until $Z=Z_{\rm min}=4$ . The network of reactions below pressure P=4.624 $\times$ 10³⁰ dyn cm^-2 is the same as in the Table A.1.
Table A.3: Non-equilibrium processes in the crust of an accreting neutron stars assuming that the X-ray ashes consist of pure $^{56}{\rm Fe}$ .
Table A.4: Nuclear processes and released heat in the inner crust, assuming initial ashes of pure $^{56}{\rm Fe}$ (i.e. as in Table A.3) but suppressing pycnonuclear fusion until $Z=Z_{\rm min}=4$ . The network of reactions below pressure P=2.637 $\times$ 10³⁰ dyn cm^-2 is the same as in Table A.3.