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The Initial Mass Function in Disc Galaxies and in Galaxy Clusters: The Chemo-Photometric Picture

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The Initial Mass Function 50 Years Later

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 327))

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Abstract

The observed brightness of the Tully-Fisher relation suggests a low stellar M/L ratio and a “bottom-light” IMF in disc galaxies, but the corresponding efficiency of chemical enrichment tends to exceed the observational estimates. Either suitable tuning of the IMF slope and mass limits or metal outflows from disc galaxies must then be invoked.

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Portinari, L. (2005). The Initial Mass Function in Disc Galaxies and in Galaxy Clusters: The Chemo-Photometric Picture. In: Corbelli, E., Palla, F., Zinnecker, H. (eds) The Initial Mass Function 50 Years Later. Astrophysics and Space Science Library, vol 327. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-3407-7_42

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