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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S321(11), p. 126

DOI: 10.1017/s1743921316009054

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Redshift evolution of Tully-Fisher relation

Journal article published in 2016 by Ismael Ferrero ORCID, Mario G. Abadi ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractUsing the eagle cosmological simulation of galaxy formation we test the ability of the ΛCDM cosmological model to reproduce the Tully-Fisher relation (TFR) and its redshift evolution. We find that our simulated galaxies follow a TFR that is in good agreement with observed results up to z = 1, indicating no evolution in the slope and a weak decrease in the zero-point.