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Home All issues Volume 508 / No 2 (December III 2009) A&A, 508 2 (2009) 565-574 Full HTML
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Table 6:

Supernovae type Ia fraction, $f = {\rm SNIa}/({\rm SNIa+SNcc})$, obtained for different theoretical SNe models from the observed Si/Fe and Ni/Fe abundance ratios. SNIa and SNcc models are the same as in Table 5.
mekal model       SNIa      
SNcc W7 W70 WDD1 WDD2 WDD3 CDD1 CDD2
No06,S 0.117-0.136 0.110-0.244          
No06,T 0.139-0.141 0.132-0.272          
CL04,S   0.149-0.193   0.168-0.384 0.134-0.289   0.154-0.348
CL04,T   0.182-0.320   0.204-0.313 0.165-0.327   0.188-0.302
W95,S     0.207-0.254 0.129-0.322 0.102-0.237 0.226-0.239 0.118-0.289
W95,T       0.143-0.338 0.113-0.250   0.131-0.304

apec model

       SNIa      
SNcc W7 W70 WDD1 WDD2 WDD3 CDD1 CDD2
No06,S   0.096-0.109   0.107-0.270 0.086-0.200   0.098-0.243
No06,T       0.130-0.301 0.104-0.225   0.119-0.272
CL04,S     0.221-0.606 0.144-0.345 0.174-0.262 0.239-0.517 0.133-0.313
CL04,T     0.269-0.543 0.179-0.388 0.145-0.300 0.290-0.453 0.166-0.354
W95,S     0.172-0.556 0.197-0.286   0.186-0.564 0.189-0.258
W95,T     0.191-0.574 0.147-0.301   0.207-0.517 0.141-0.272


Source LaTeX | All tables | In the text

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