Table 2: The stellar yields (expressed in solar masses) as derived in this paper, namely those that produce the best agreement with observations.

)	K	Sc	Ti	Cr	Mn	Co	Ni
11.00	.4040E-04	.2564E-05	.3300E-03	.2037E-02	.1290E-03	.1272E-03	.1670E-01
12.00	.1712E-02	.2714E-05	.3960E-03	.2091E-02	.1400E-03	.2010E-04	.7000E-02
13.00	.6160E-04	.2553E-05	.3990E-03	.1929E-02	.4490E-03	.2019E-04	.1120E-01
15.00	.2544E-03	.6751E-05	.7515E-03	.1371E-02	.4710E-03	.3030E-04	.6800E-02
18.00	.1176E-03	.2415E-05	.8400E-03	.8910E-03	.4040E-03	.4290E-04	.3760E-02
19.00	.6952E-03	.6038E-05	.8670E-03	.7980E-03	.2060E-03	.7710E-04	.4680E-02
20.00	.7496E-03	.1086E-04	.8700E-03	.5400E-03	.2130E-03	.8160E-04	.4440E-02
22.00	.1200E-02	.2530E-04	.8940E-04	.4050E-03	.2300E-03	.8820E-04	.1120E-01
25.00	.4032E-03	.2622E-05	.7500E-04	.3900E-03	.2580E-03	.7500E-03	.7590E-02
30.00	.2648E-03	.1610E-05	.1500E-03	.4500E-03	.1040E-03	.8070E-03	.3350E-01
35.00	.1328E-03	.1345E-05	.4500E-03	.4500E-03	.1330E-03	.7950E-03	.2040E-02
40.00	.8960E-04	.1621E-05	.4560E-03	.9120E-04	.1340E-03	.8250E-03	.2120E-02
50.00	.8960E-04	.1621E-05	.4560E-03	.6120E-04	.1340E-03	.8250E-03	.2120E-02
60.00	.8960E-04	.1621E-05	.4560E-03	.3120E-04	.1340E-03	.8250E-03	.2120E-02
70.00	.8960E-04	.1621E-05	.4560E-03	.3120E-04	.1340E-03	.8250E-03	.2120E-02
80.00	.8960E-04	.1621E-05	.4560E-03	.3120E-04	.1340E-03	.8250E-03	.2120E-02
90.00	.8960E-04	.1621E-05	.4560E-03	.3120E-04	.1340E-03	.8250E-03	.2120E-02
100.00	.8960E-04	.1621E-05	.4560E-03	.3120E-04	.1340E-03	.8250E-03	.2120E-02