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

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Table 2

Same as Table 1, but considering 2D SNIa models instead of the 1D Classical SNIa models.

SNcc	SNIa						χ²/ d.o.f.


Nomoto	2D	−	−

Z0.02	O-DDT			0.35	−	−	56.0/8
Z0.001	O-DDT			0.41	−	−	60.0/8
Z0.008	O-DDT			0.37	−	−	63.1/8
Z0.004	O-DDT			0.39	−	−	69.0/8
Z0.008	C-DEF			0.36	−	−	79.9/8

Nomoto	2D	Ca-rich gap	−

Z0.02	O-DDT	CO.5HE.2C.3^(*)		0.39	0.10	−	30.2/7
Z0.001	O-DDT	CO.5HE.2C.3^(*)		0.45	0.09	−	32.7/7
Z0.02	C-DEF	CO.5HE.2C.3^(*)		0.38	0.09	−	36.8/7
Z0.008	O-DDT	CO.5HE.2C.3^(*)		0.41	0.09	−	39.5/7
Z0.008	C-DEF	CO.5HE.2C.3^(*)		0.40	0.08	−	40.1/7

Nomoto	2D	2D	Ca-rich gap

Z0.02	C-DEF	O-DDT	CO.5HE.2C.3^(*)	0.39	0.10	0.13	26.3/6
Z0.001	C-DEF	O-DDT	CO.5HE.2C.3^(*)	0.45	0.09	0.07	30.3/6
Z0.008	C-DEF	O-DDT	CO.5HE.2C.3^(*)	0.41	0.09	0.16	33.9/6
Z0.004	C-DEF	O-DDT	CO.5HE.2C.3^(*)	0.43	0.08	0.18	39.9/6
Z0.02	C-DEF	C-DDT	CO.5HE.2C.3^(*)	0.40	0.09	0.79	41.9/6

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