Boron in Orion: Cycle 3 Medium

Details Boron in Orion: Cycle 3 Medium Boron in Orion: Cycle 3 Medium

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4573g&link_type=abstract

HST Proposal ID #4573

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Hst Proposal Id #4573

Scientific paper

The abundance of Boron will be derived from the B II 1362A resonance line for a sample of massive (8-9 Msun) stars. Stars near the Trapezium in Orion are enriched in Oxygen. This enrichment is presumed to be due to enrichment of the parental molecular cloud with Oxygen from SNeII. If B is synthesized by neutrino-induced spallation in SNeII, the O-rich Orion stars will be overabundant in Boron. This prediction will be tested by measuring the 1362A line in the most O-rich Orion star, and by comparing the Boron abundance with that for other O-normal Orion stars.

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