Metal abundances in the cool cores of galaxy clusters

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Volume 508 / No 2 (December III 2009)

A&A, 508 2 (2009) 565-574

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Table A.1:

Yields of elements in solar masses for different SNe models. Type Ia yields were calculated for each element for the W7, W70, WDD1, WDD2, WDD3 and CDD1, CDD2 models in Iwamoto et al. (1999). SN core-collapsed yields (including types Ib and Ic) were calculated from the results in Nomoto et al. (2006) integrating over a progenitor initial mass function. We have considered two different initial mass functions, the Salpeter function with index 1.35 and the AY top-heavy function with index 0.95, and we have integrated between 10 and 50 solar masses. The initial metallicity of the progenitors is Z=0.02 (i.e. solar).
SNIa
Element	W7	W70	WDD1	WDD2	WDD3	CDD1	CDD2
Si	0.16	0.14	0.27	0.21	0.16	0.28	0.20
Fe	0.76	0.77	0.67	0.79	0.87	0.65	0.83
Ni	0.13	0.10	0.04	0.06	0.07	0.04	0.06

SNcc
Element	Nomoto etal. (2006)		Chieffi & Limongi (2004)		Woosley & Weaver (1995)
	Salpeter	top-heavy	Salpeter	top-heavy	Salpeter	top-heavy
Si	0.113	0.124	0.163	0.183	0.127	0.132
Fe	0.090	0.091	0.132	0.135	0.109	0.106
Ni	0.005	0.005	0.014	0.013	0.014	0.013

Source LaTeX | All tables | In the text

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