2003/01/03 by Nikos Prantzos, Prantzos, Nikos
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0301043
10 pages, 6 figs; Invited review talk in the Conference "CNO in the Universe" (St. Luc, Switzerland, Sept. 2002), Eds. C. Charbonnel, G. Meynet and D. Schaerer, ASP Conf. series, in press
arxiv created 2003/01/03 · arxiv updated 2009/12/01
After summarizing the most important features of current stellar yields of CNO elements (including recent results concerning rotating and mass losing stars) I discuss how these yields may help to interpret relevant observations in the local Galaxy, the Milky Way disk and extragalactic systems (extragalactic HII regions and DLAs).