Abstract
We have computed chemical evolution models for a sample of local dSph galaxies (Carina, Draco, Leol, Leoll, and Ursa Minor) based on their star formation histories (S F H HGV ) as inferred from observed HR diagrams by Hernández, Gilmore, and Valls-Gabaud (2000).
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References
Carigi, L., Hernandez, X. and Gilmore, G.: 2001, Mon. Not. R. Astron. Soc.,submitted.
Hernandez, X., Gilmore, G. and Valls-Gabaud, D.: 2000, Mon. Not. R. Astron. Soc. 317, 831.
Mateo, M.: 1998, Annual Review Astron. Astrophys. 36, 435.
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© 2001 Springer Science+Business Media Dordrecht
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Carigi, L., Gilmore, G., Hernández, X. (2001). Chemical Evolution Models of Local dSph Galaxies. In: Vílchez, J.M., Stasińska, G., Pérez, E. (eds) The Evolution of Galaxies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3313-7_42
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DOI: https://doi.org/10.1007/978-94-017-3313-7_42
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