Abstract
Stellar models with axial rotation and very low metallicity Z, typical of the early star generations have been computed. These models account for the effects of rotation in the same way as previous grids which successfully reproduce the He- and N-enrichments observed at the surface of massive stars, and also the high numbers of red supergiants observed in low Z galaxies (Meynet and Maeder, 2000; Maeder and Meynet, 2001). At very low metallicity (Z = 0.00001, i.e. one two thousandth of the solar metallicity), these models naturally lead to the production of primary nitrogen.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Edmunds, M.G. and Pagel, B.E.J.: 1978, MNRAS 185, 77.
Garnett, D.R. et al.: 1997, ApJ 489, 63.
Langer, N., Heger, A., Wellstein, S. and Herwig, F.: 1999, A&A 346, L37.
Maeder, A., Grebel, E. and Mermilliod, J.C.: 1999, A&A 346, 459.
Maeder, A. and Meynet, G.: 2001, A&A 373, 555.
Meynet, G. and Maeder, A.: 2000, A&A 361, 101.
Talbot, R.J. and Arnett, W.D.: 1974, ApJ 190, 605.
Thuan, T.X., Izotov, Y.I. and Lipovetsky, V.A.: 1995, ApJ 445, 108.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2002 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Meynet, G. (2002). Primary Nitrogen Production at Low Z. In: Sauvage, M., Stazińska, G., Schaerer, D. (eds) The Evolution of Galaxies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3311-3_32
Download citation
DOI: https://doi.org/10.1007/978-94-017-3311-3_32
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-6020-4
Online ISBN: 978-94-017-3311-3
eBook Packages: Springer Book Archive