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Stellar populations in bulges: the isolated galaxies

Authors: Morelli, L.; Costantin, L.; Corsini, E. M.; Dalla Bontà, E.; Coccato, L.; Méndez-Abreu, J.; Pizzella, A.;

Stellar populations in bulges: the isolated galaxies

Abstract

En una reciente serie de artículos se han presentado los resultados de la investigación sobre la población estelar y sus gradientes en las regiones de la galaxias donde la luz esta dominada por el bulbo. En la presentación oral se han mostrado los resultados de estos trabajos y los últimos avances del proyecto, mostrando las propriedades de la población estelar en el bulbo de galaxias en ambiente aislado.

In a recent series of papers we presented the results of the investigation on the stellar populations and their gradients of the bulge dominated region. The results of these works have been presented in the talk along with the last progresses in this projects, showing the properties of the stellar populations in the bulge dominated regions of galaxies in isolated environment.

Asociación Argentina de Astronomía

Countries
Italy, Argentina
Keywords

570, Ciencias Astronómicas, galaxies: spiral, galaxies: stellar content, galaxies: formation, galaxies: abundances, 530, galaxies: bulges, galaxies: kinematics and dynamics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green