Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.7608h&link_type=abstract
American Astronomical Society, 197th AAS Meeting, #76.08; Bulletin of the American Astronomical Society, Vol. 32, p.1525
Astronomy and Astrophysics
Astronomy
Scientific paper
We employ analytical and numerical chemical evolution models to interpret observed trends in abundance ratios involving carbon, nitrogen, and oxygen. Several sets of published stellar yields for both intermediate-mass and massive stars are considered, and the most appropriate sets are selected through the use of the analytical models. These yields are then used in the numerical models to match observed data trends in C/O, N/O, and O/H. We conclude that the principal production site for carbon is massive stars, while that for nitrogen is intermediate-mass stars.
Edmunds Michael G.
Henry Richard B. C.
Köppen Joachim
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