a References: solar system data: Canyon Diablo troilite (CDT),
Ding et al. (2001); ISM data: Chin et al.
(1996), Mauersberger et al. (1996), most
ISM data are from the inner Galaxy; Cosmic Rays: these are
"source abundances'', Thayer (1997); IRC+10216: Kahane
et al. (2000), this paper.
b The average value for
sources at various galactocentric radii; the data by Chin et al.
(1996) indicate a possible galactocentric
32S/34S abundance gradient, which would correspond to a
value of 32( )
at the solar circle.
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