C, N, Si, Fe, Sr, Zr, Mo and Ba Isotopic Analyses of Type X Murchison SiC Grains: Experimental Evidence for a New Type of Stellar Nucleosynthesis in Supernovae

Details C, N, Si, Fe, Sr, Zr, Mo and Ba Isotopic Analyses of Type X Murchison SiC Grains: Experimental Evidence for a New Type of Stellar Nucleosynthesis in Supernovae C, N, Si, Fe, Sr, Zr, Mo and Ba Isotopic Analyses of Type X Murchison SiC Grains: Experimental Evidence for a New Type of Stellar Nucleosynthesis in Supernovae

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002m%26psa..37q.115p&link_type=article

Meteoritics & Planetary Science, vol. 37, Supplement, p.A115

Physics

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

C, N, Si, Fe, Sr, Zr, Mo and Ba Isotopic Analyses of Type X Murchison SiC Grains: Experimental Evidence for a New Type of Stellar Nucleosynthesis in Supernovae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with C, N, Si, Fe, Sr, Zr, Mo and Ba Isotopic Analyses of Type X Murchison SiC Grains: Experimental Evidence for a New Type of Stellar Nucleosynthesis in Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and C, N, Si, Fe, Sr, Zr, Mo and Ba Isotopic Analyses of Type X Murchison SiC Grains: Experimental Evidence for a New Type of Stellar Nucleosynthesis in Supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-735505