Chempy: A flexible chemical evolution model for abundance fitting - Do the Sun’s abundances alone constrain chemical evolution models?

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Table 2

Yield sets for which we test our inference.


Yield set	CC-SN	SN Ia	AGB


Default	Nomoto et al. (2013) (net)^a	Seitenzahl et al. (2013)	Karakas (2010) (net)^a
Alternative	Chieffi & Limongi (2004) (gross)^b	Thielemann et al. (2003)	Ventura et al. (2013) (net)^a

Notes.

^(a)

“Net” means that the original yield tables provide only the newly produced material; any material that was originally present in the star and expelled into the ISM without further processing is computed by us according to the chemical composition of the ISM at the star’s birth predicted by our GCE model.

^(b)

“Gross” means that we are using the total (newly produced + unprocessed) stellar ejecta provided in the original yield tables.

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