A tectonic model for the Tertiary evolution of strike–slip by C.K. Morley

By C.K. Morley

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Data sources: Hoppe et al. (1994, 1996a, 1996b, 1997, 2000), Nittler et al. (1995), Gao and Nittler (1997), Huss et al. (1997), Amari et al. (2001a, 2001b, 2001c), and Nittler and Hoppe (2005) (ii) The AGB star-specific signature of s-process nucleosynthesis is seen in the isotopic patterns of intermediate-mass to heavy elements. (iii) SiC is observed in stellar spectra (see Molster and Waters 2002). (iv) Carbon stars are the most prolific injectors of dust into the ISM (see Gail 2002). 1 Mainstream Grains The mainstream grains have 12 C/ 13 C ratios between 10 and 200 and 14 N/ 15 N ratios between 50 and 20,000 (Fig.

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