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- W2022715089 abstract "Galaxy number counts at faint magnitudes exceed the expectations from non-evolving models, based on the present-day galaxy population, by a large margin. Despite this, redshift surveys show that the redshift distribution is as expected in the non-evolving case, lacking in particular the tail of evolved bright galaxies at high z predicted by the standard evolutionary models. We consider here the effect of using a broadly peaked, rather than steadily rising, luminosity evolution model. Evolution of this form has as its physical basis current infall models for the history of star formation in our galaxy" @default.
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- W2022715089 date "1993-07-01" @default.
- W2022715089 modified "2023-09-23" @default.
- W2022715089 title "Infall models of galaxy evolution: a solution to the redshift distribution problem?" @default.
- W2022715089 doi "https://doi.org/10.1093/mnras/263.1.86" @default.
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