The Source of Cosmic Rays: 1. Be/Fe Evolution and Cosmic Ray Composition

Details The Source of Cosmic Rays: 1. Be/Fe Evolution and Cosmic Ray Composition The Source of Cosmic Rays: 1. Be/Fe Evolution and Cosmic Ray Composition

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4..140r&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

Be abundance observations in old halo stars formed in the early Galaxy
have opened a new channel in cosmic-ray origin studies. The essentially
constant ratio of Be-to-Fe abundance as a function of the Fe abundance
of the stars strongly suggests that the bulk of the cosmic rays metals
are accelerated out of fresh supernova ejecta.

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