Cumulative isotopic yields |
| Mass (in solar masses) |
|
13 |
15 |
20 |
25 |
30 |
35 |
Z = 0 |
|
|
|
|
|
|
Z = 1e-6 |
|
|
|
|
|
|
Z = 1e-4 |
|
|
|
|
|
|
Z = 1e-3 |
|
|
|
|
|
|
Z = 6e-3 |
|
|
|
|
|
|
Z = 2e-2 |
|
|
|
|
|
|
READ ME
Each row contains the yields integrated (in Msun) from the surface up to that specific mass layer. All the unstable nuclei are fully
decayed to their stable daughter in advance. For each mass there are 12 files, 11 from zxxmxx.q10 to zxxmxx.q20 and a file called
zxxmxx.nik. The legenda of the various columns is in the first row of each file. For convenience each file has the mass (in Msun) in
the first column. The .nik file contain the cumulative abundance (in solar masses) of the Ni56 so that it is easy to find the mass
cut corresponding to each specific amount of Ni56 ejected outward. The meaning of the filenames is as follows: Zxx refers the
metallicity: z13=0.001, z63=0.006 and so on. Mxx refers to the star mass in solar masses.