Some caveats about the evolution of the N/O abundance and the star formation history

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics

Scientific paper

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6 pages, 7 fig. Proceedings of the 10th Torino workshop on AGB nucleosynthesis, Eds. C. Worley, C. Tout and R. Stancliffe

Scientific paper

We carefully analyze how the abundance of Nitrogen over Oxygen evolves when dependent on metallicity stellar yields with a primary component of N proceeding from AGBs stars are used. We show the results obtained with a chemical evolution models grid, calculated with variable star formation efficiencies, which produce different star formation histories. Finally we see how the N/O abundance is related on the evolutionary history.

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