The tully-fisher relation in numerical simulations of structure formation

María E. De Rossi, Patricia B. Tissera, Susana E. Pedrosa

Resultado de la investigación: Article

Resumen

The Tully-Fisher Relation (TFR) is of fundamental importance for galaxy formation as it provides information about the relation between the baryonic content of galaxies and the depth of their dark halos potential wells. In recent years, it has been possible to study this relation at different redshifts. However, there are still controversies about its origin and evolution. In this work, we try to address the origin of the Tully-Fisher Relation by employing cosmological hydrodynamical simulations.

Idioma originalEnglish
Páginas (desde-hasta)327-328
Número de páginas2
PublicaciónProceedings of the International Astronomical Union
Volumen5
N.ºS262
DOI
EstadoPublished - 1 ago 2009

Huella dactilar

Tully-Fisher relation
well
galactic evolution
simulation
halos
galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Citar esto

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The tully-fisher relation in numerical simulations of structure formation. / De Rossi, María E.; Tissera, Patricia B.; Pedrosa, Susana E.

En: Proceedings of the International Astronomical Union, Vol. 5, N.º S262, 01.08.2009, p. 327-328.

Resultado de la investigación: Article

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AU - Pedrosa, Susana E.

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KW - Galaxies: evolution

KW - Galaxies: formation

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