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

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 ind...

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Bibliographic Details
Published in:arXiv.org 2010-05
Main Authors: M Fernández Lorenzo, Cepa, J, Bongiovanni, A, Pérez García, A M, Lara-López, M A, Pović, M, Sánchez-Portal, M
Format: Article
Language:English
Subjects:
Astronomical models
Cosmology
Galactic evolution
Galactic rotation
Image classification
Image detection
Line spectra
Luminosity
Morphology
Photometry
Red shift
Spiral galaxies
Star & galaxy formation
Star formation
Stellar evolution
Stellar populations
Tully-Fisher relation
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Summary: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
ISSN:2331-8422
DOI:10.48550/arxiv.1005.1512