Elemental Ratios of Light Elements Synthesized in Supernovae

Details Elemental Ratios of Light Elements Synthesized in Supernovae Elemental Ratios of Light Elements Synthesized in Supernovae

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000asthe..93..673y&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 93, No. 11, p. 673 - 679 (2000)

Astronomy and Astrophysics

Astronomy

Scientific paper

In meteorites there are presolar grains which have their isotopic ratios indicating the nucleosynthesis in their birth. Comparing the isotopic ratios in the grains with those obtained by nucleosynthesis theories, we identify the origin of the presolar grains. In order to identify presolar grains originated from supernovae, the author investigates available regions of the isotopic/elemental ratios of rare light elements (Li, Be, B) and the CNO-elements produced in the He-layer and the H-rich envelope in supernovae.

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