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Stellar Population Gradients in Phoenix and Leo I

Published online by Cambridge University Press:  25 May 2016

D. Martínez-Delgado ,
Carme Gallart ,
A. Aparicio  and
W. Freedman
D. Martínez-Delgado
Affiliation:
Instituto de Astrofísica de Canarias, E38200 La Laguna, Tenerife, Canary Islands, Spain
Carme Gallart
Affiliation:
Carnegie Observatories, Pasadena CA91101, USA
A. Aparicio
Affiliation:
Instituto de Astrofísica de Canarias, E38200 La Laguna, Tenerife, Canary Islands, Spain
W. Freedman
Affiliation:
Carnegie Observatories, Pasadena CA91101, USA

Abstract

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The study of gradients in the stellar populations of dwarf galaxies will give us necessary information to construct detailed models of their formation and evolution. We find clear traces of these gradients, in the sense of stars being older for larger galactocentric distances, in two interesting nearby dwarfs: Phoenix and Leo I.

Type
Part 3: Star Formation Processes and Chemical Evolution
Information
Symposium - International Astronomical Union , Volume 192: The Stellar Content of Local Group Galaxies , 1999 , pp. 325 - 329
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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