Origin of central abundances in the hot intra-cluster medium - II. Chemical enrichment and supernova yield models

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Table 3

Same as Table 1, but considering 3D SNIa models instead of the 1D Classical SNIa models.

SNcc	SNIa						χ²/ d.o.f.


Nomoto	3D	−	−

Z0.008	N100H			0.26	−	−	47.2/8
Z0.004	N100H			0.28	−	−	47.3/8
Z0.02	N100H			0.25	−	−	49.8/8
Z0.001	N100H			0.30	−	−	55.1/8
Z0.02	N150			0.31	−	−	55.6/8

Nomoto	3D	Ca-rich gap	−

Z0.02	N100H	CO.5HE.2C.3^(*)		0.31	0.17	−	11.8/7
Z0.008	N100Hdef	CO.5HE.2C.3^(*)		0.44	0.11	−	12.0/7
Z0.02	N100Hdef	CO.5HE.2C.3^(*)		0.43	0.12	−	12.8/7
Z0.004	N100Hdef	CO.5HE.2C.3^(*)		0.45	0.10	−	12.9/7
Z0.008	N100H	CO.5HE.2C.3^(*)		0.32	0.15	−	13.1/7

Nomoto	3D	3D	Ca-rich gap

Z0.008	N100Hdef	N100H	CO.5HE.2C.3^(*)	0.42	0.11	0.77	11.2/6
Z0.02	N100Hdef	N150	CO.5HE.2C.3^(*)	0.41	0.12	0.69	11.3/6
Z0.02	N100Hdef	N100L	CO.5HE.2C.3^(*)	0.43	0.11	0.76	11.4/6
Z0.02	N100Hdef	N100	CO.5HE.2C.3^(*)	0.41	0.12	0.75	11.6/6
Z0.02	N100Hdef	N100H	CO.5HE.2C.3^(*)	0.40	0.12	0.76	11.7/6

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