DOI: 10.5281/zenodo.14981332
title: Online material for 'Impact of $\textit{T}$- and $\rho$-dependent decay rates and new (n,$\gamma$) cross sections on the $\textit{s}$ process in low-mass asymptotic giant branch stars'

description: Online material for the article titled 'Impact of $\textit{T}$- and $\rho$-dependent decay rates and new (n,$\gamma$) cross sections on the $\textit{s}$ process in low-mass AGB stars'.

Files:



srf.tar.gz: Surface isotopic abundance data tables of seven stellar models of low-mass AGB stars from Karakas & Lugaro (2016) for three nuclear networks. The sources of the reaction rates in the different sets are described in Table 2 of the article. Each file includes 1) The essential features of the models in the header: initial mass (M), initial mass fraction of helium (Y), initial metallicity (Z), and the nucleosynthesis set; 2) The mass number (A), atomic number (Z) and neutron number (N) for 328 isotopes that includes in our nuclear network; 3) Initial normalised number abundances (from Apslund et. al. 2009) used in the post-processing calculations; 4) Surface normalised number abundances calculated at each thermal pulse steps; 5) Final normalised number abundances computed at the last time step.




Filename
Mass ($\mathrm{M_{\odot}}$)
Metallicity
Set


srf_m3z007_set0.dat
3
0.007
0


srf_m4z007_set0.dat
4
0.007
0


srf_m2z014_set0.dat
2
0.014
0


srf_m3z014_set0.dat
3
0.014
0


srf_m4z014_set0.dat
4
0.014
0


srf_m3z030_set0.dat
3
0.03
0


srf_m4z030_set0.dat
4
0.03
0


srf_m3z007_set1.dat
3
0.007
1


srf_m4z007_set1.dat
4
0.007
1


srf_m2z014_set1.dat
2
0.014
1


srf_m3z014_set1.dat
3
0.014
1


srf_m4z014_set1.dat
4
0.014
1


srf_m3z030_set1.dat
3
0.03
1


srf_m4z030_set1.dat
4
0.03
1


srf_m3z007_set2.dat
3
0.007
2


srf_m4z007_set2.dat
4
0.007
2


srf_m2z014_set2.dat
2
0.014
2


srf_m3z014_set2.dat
3
0.014
2


srf_m4z014_set2.dat
4
0.014
2


srf_m3z030_set2.dat
3
0.03
2


srf_m4z030_set2.dat
4
0.03
2











sy.tar.gz: Stellar yield data tables of seven stellar models of low-mass AGB stars from Karakas & Lugaro (2016) for three nuclear networks. The sources of the reaction rates in the different sets are described in Table 2 of the article. Each file includes 1) The essential features of the models in the header: initial mass (M), initial mass fraction of helium (Y), initial metallicity (Z), and the nucleosynthesis set; 2) The mass number (A), atomic number (Z) and neutron number (N) for 328 isotopes that includes in our nuclear network; 3) Stellar yields expressed in units of solar mass calculated by the method described in Section 2.3 of the article.




Filename
Mass ($\mathrm{M_{\odot}}$)
Metallicity
Set


sy_m3z007_set0.dat
3
0.007
0


sy_m4z007_set0.dat
4
0.007
0


sy_m2z014_set0.dat
2
0.014
0


sy_m3z014_set0.dat
3
0.014
0


sy_m4z014_set0.dat
4
0.014
0


sy_m3z030_set0.dat
3
0.03
0


sy_m4z030_set0.dat
4
0.03
0


sy_m3z007_set1.dat
3
0.007
1


sy_m4z007_set1.dat
4
0.007
1


sy_m2z014_set1.dat
2
0.014
1


sy_m3z014_set1.dat
3
0.014
1


sy_m4z014_set1.dat
4
0.014
1


sy_m3z030_set1.dat
3
0.03
1


sy_m4z030_set1.dat
4
0.03
1


sy_m3z007_set2.dat
3
0.007
2


sy_m4z007_set2.dat
4
0.007
2


sy_m2z014_set2.dat
2
0.014
2


sy_m3z014_set2.dat
3
0.014
2


sy_m4z014_set2.dat
4
0.014
2


sy_m3z030_set2.dat
3
0.03
2


sy_m4z030_set2.dat
4
0.03
2