RMxAA

Revista Mexicana de Astronomía y Astrofísica

ISSN: 3061-8649
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Chemical evolution of galaxies. III.. The N/O versus O/H relationship. (1983). Revista Mexicana De Astronomía Y Astrofísica, 8(1), 117-129. https://astronomia.unam.mx/journals/rmxaa/article/view/1983rmxaa...8..117s

Abstract

The N/O, 0/H diagram derived from galactic and extragalactic H II regions can be explained under the assumptions that most of the N is of secondary origin, that most of the N is produced by intermediate mass stars (1 M/M® S), and that accretion plays an important role in the chemical evolution of galaxies. Several observational and theoretical arguments are presented in favor of these hypotheses. Given that constant-yield models can never reach 12 + log 0/H % 9.0 because the instantaneous recycling for 0, breaks down it is an essential component of the new model that the yield increases with metallicity.
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