Beryllium production in early Galactic history

Beryllium production in early Galactic history

It is suggested that, if most star formation in the Galactic halo occurred in objects the size of globular clusters, then most of the spallation reactions producing beryllium could also have occurred in such objects, and that this could have led to the observed approximately linear relationship betw...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 1995-03, Vol.273 (1), p.215-218
1. Verfasser: Tayler, R. J.
Format: Artikel
Sprache:eng
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abundances
cosmic rays
Galaxy: abundances
Galaxy: halo
nuclear reactions
nucleosynthesis
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container_title Monthly notices of the Royal Astronomical Society
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creator Tayler, R. J.
description It is suggested that, if most star formation in the Galactic halo occurred in objects the size of globular clusters, then most of the spallation reactions producing beryllium could also have occurred in such objects, and that this could have led to the observed approximately linear relationship between beryllium and oxygen abundances. Furthermore, it is plausible that the relative spallation rates in the halo and the disc could lead to the beryllium-oxygen relationship observed at higher metallicities.
doi_str_mv 10.1093/mnras/273.1.215
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source Oxford Journals Open Access Collection; EZB-FREE-00999 freely available EZB journals; Oxford University Press Journals Digital Archive Legacy
subjects abundances
cosmic rays
Galaxy: abundances
Galaxy: halo
nuclear reactions
nucleosynthesis
title Beryllium production in early Galactic history
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