The Gaia-ESO survey: galactic evolution of sulphur and zinc
Due to their volatile nature, when sulfur and zinc are observed in external galaxies, their determined abundances represent the gas-phase abundances in the interstellar medium. This implies that they can be used as tracers of the chemical enrichment of matter in the Universe at high redshift. Compar...
Gespeichert in:
| Hauptverfasser: | , , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
2017
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| In: |
Arxiv
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| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1704.02981
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| Verfasserangaben: | S. Duffau, E. Caffau, L. Sbordone, P. Bonifacio, S. Andrievsky, S. Korotin, C. Babusiaux, S. Salvadori, L. Monaco, P. François, Á Skúladóttir, A. Bragaglia, P. Donati, L. Spina, A.J. Gallagher, H.-G. Ludwig, N. Christlieb, C.J. Hansen, A. Mott, M. Steffen, S. Zaggia, S. Blanco-Cuaresma, F. Calura, E. Friel, F.M. Jiménez-Esteban, A. Koch, L. Magrini, E. Pancino, B. Tang, G. Tautvaišienė, A. Vallenari, K. Hawkins, G. Gilmore, S. Randich, S. Feltzing, T. Bensby, E. Flaccomio, R. Smiljanic, A. Bayo, G. Carraro, A.R. Casey, M.T. Costado, F. Damiani, E. Franciosini, A. Hourihane, P. Jofré, C. Lardo, J. Lewis, L. Morbidelli, S.G. Sousa, and C.C. Worley |
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