Evolution of the infrared Tully-Fisher relation up to z=1.4

Details Evolution of the infrared Tully-Fisher relation up to z=1.4 Evolution of the infrared Tully-Fisher relation up to z=1.4

2010-05-10

arxiv.org/abs/1005.1512v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

14 pages, 10 figures; accepted in A&A

Scientific paper

The Tully-Fisher relation (TFR) represents a connection between fundamental galaxy parameters, such as its total mass and the mass locked in stars. Therefore, the study of the evolution of this relation in the optical and infrared bands can provide valuable information about the evolution of the individual galaxies through the changes found in each band. This work aims to study the TFR at high redshift in the B, V, R, I, and K-bands by comparison with the local relations derived from a large sample of galaxies in the redshift range 0.1

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