Bibcode
Méndez-Abreu, J.; Aguerri, J. A. L.; Corsini, E. M.
Referencia bibliográfica
Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at the Centro Convegni Matteo Ricci, Rome, Italy. Edited by José G. Funes, S.J., and Enrico Maria Corsini. San Francisco: Astronomical Society of the Pacific, 2008., p.369
Fecha de publicación:
10
2008
Número de citas
1
Número de citas referidas
1
Descripción
We studied the fraction and properties of bars in a sample of about 3000
galaxies extracted from SDSS-DR5. This represents a volume limited
sample with galaxies located between redshift 0.01-20, and inclination i < 60°.
Interacting galaxies were excluded from the sample. The fraction of
barred galaxies in our sample is 45%. We found that 32% of S0s, 55% of
early-type spirals, and 52% of late-type spirals are barred galaxies.
The bars in S0s galaxies are weaker than those in later-type galaxies.
The bar length and galaxy size are correlated, being larger bars located
in larger galaxies. Neither the bar strength nor bar length correlate
with the local galaxy density. On the contrary, the bar properties
correlate with the properties of their host galaxies. Galaxies with
higher central light concentration host less and weaker bars.
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Casiana
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