Table 1:
Yields produced in low and intermediate stars for solar metallicity.
|
Mass |
H |
He |
C12 |
N14 |
O16 |
C13 |
C12P |
N14P |
O16P |
C13P |
![$\rm [Fe/H]=0.0$](/articles/aa/full/2005/12/aa1949/img70.gif) |
| 1.00 |
-0.13E-01 |
0.13E-01 |
-0.35E-03 |
0.40E-03 |
-0.42E-04 |
0.30E-04 |
0.00E+00 |
0.00E+00 |
0.00E+00 |
0.00E+00 |
| 1.10 |
-0.14E-01 |
0.14E-01 |
-0.42E-03 |
0.50E-03 |
-0.51E-04 |
0.36E-04 |
0.00E+00 |
0.00E+00 |
0.00E+00 |
0.00E+00 |
| 1.20 |
-0.16E-01 |
0.16E-01 |
-0.51E-03 |
0.59E-03 |
-0.59E-04 |
0.42E-04 |
0.00E+00 |
0.00E+00 |
0.00E+00 |
0.00E+00 |
| ... |
... |
... |
... |
... |
... |
.... |
.... |
.... |
.... |
.... |
| 8.00 |
-0.55E+00 |
0.54E+00 |
-0.16E-01 |
0.42E-01 |
-0.18E-01 |
0.47E-03 |
0.24E-02 |
0.56E-02 |
0.15E-03 |
0.14E-03 |
Source LaTeX |
All tables |
In the text
