Nucleosynthesis of solar system matter

Details Nucleosynthesis of solar system matter Nucleosynthesis of solar system matter

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.2034l&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Astronomy and Astrophysics

Astrophysics

Energetic Particles, Interplanetary Space, Nuclear Astrophysics, Nuclear Fusion, Deuterium, Helium Isotopes, Isotope Effect, Solar System Evolution

Scientific paper

Conclusions on the nature of the most probable objects and on the number of stages of the nucleosynthesis of solar system matter are drawn on the basis of data on the role of nuclear reactions with high-energy particles. A curve of the atomic abundance of bypassed isotopes and their quantities is presented, and the sequence of the processes of the genesis of solar system matter is illustrated.

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