Table 1:
The stellar yields (expressed in solar masses) as derived in this paper, namely those that produce the best
agreement with observations. Yields for O are identical to metal dependent yields of WW95.
 ) |
Mg |
Si |
Ca |
Fe |
Zn |
| 11.00 |
.6440E-01 |
.2170E-01 |
.1400E-02 |
.8000E-01 |
.3510E-04 |
| 12.00 |
.5740E-01 |
.9090E-01 |
.1500E-01 |
.5500E-01 |
.3360E-04 |
| 13.00 |
.1148E+00 |
.5850E-01 |
.3600E-02 |
.1460E+00 |
.4500E-04 |
| 15.00 |
.1869E+00 |
.1100E+00 |
.1110E-01 |
.1297E+00 |
.7280E-04 |
| 18.00 |
.3864E+00 |
.1370E+00 |
.6900E-02 |
.8300E-01 |
.1060E-03 |
| 19.00 |
.1757E+00 |
.2770E+00 |
.1380E-01 |
.1170E+00 |
.1560E-03 |
| 20.00 |
.2191E+00 |
.2880E+00 |
.1480E-01 |
.1060E+00 |
.3160E-03 |
| 22.00 |
.2912E+00 |
.3560E+00 |
.1770E-01 |
.2225E+00 |
.3240E-03 |
| 25.00 |
.7000E-01 |
.3150E+00 |
.1690E-01 |
.1500E+00 |
.4070E-03 |
| 30.00 |
.7000E-01 |
.3160E+00 |
.1340E-01 |
.2500E-01 |
.3818E-03 |
| 35.00 |
.7000E-01 |
.1120E+00 |
.1600E-02 |
.2770E-01 |
.4176E-03 |
| 40.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
| 50.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
| 60.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
| 70.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
| 80.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
| 90.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
| 100.00 |
.7000E-01 |
.5460E-01 |
.1600E-02 |
.2830E-01 |
.3710E-03 |
Source LaTeX |
All tables |
In the text