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			Dear Yves,

			I send you the table with the mass ejecta for the elements O, Mg, Si, and Fe,
			plus the mass in the He_core, in the remnant and the total metal ejection.
			This table is based on the work by Fran輟is et al (2004) who changed the
			the tables by WW95 (the ones for solar metallicity) in order to best match
			the observational data at low metallicity in our Galaxy (the so-called observational yields)

			To stay in his same "scenario" I guess it is better to use his same yields for SNIa
			which are for these elements (or at least for the next future)

			QIa(3)= 0.143 ! 3)O16
			QIa(7)= 0.0425 ! 7)Mg
			QIa(8)= 0.154 ! 8)Si
			QIa(9)= 0.4 (*) ! 9)Fe


			I hope the table is fine, let me know! Of course I am ready to change format
			or, for example put the mass fraction rather than the mass.
			...then please send we the integral you obtain, just to have a cross check!

			Ciao!

			Gabriele

			(*) this is a bit weird but it is what he uses in that paper...
			I prefer the value 0.6 that is closer to the observational values.

Gear/PyChem/shared/tables/Francois/Readme
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