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Tracing stellar populations of galaxies with the SBF method

Published online by Cambridge University Press:  01 December 2006

G. Raimondo ,
M. Cantiello ,
E. Brocato ,
J. P. Blakeslee  and
M. Capaccioli
G. Raimondo
Affiliation:
INAF-Astronomical Observatory of Teramo, I-64100, Teramo, Italy email: [email protected], [email protected]
M. Cantiello
Affiliation:
Dep. of Physics and Astronomy, Washington State University Pullman, WA 99164, USA email: [email protected], [email protected]
E. Brocato
Affiliation:
INAF-Astronomical Observatory of Teramo, I-64100, Teramo, Italy email: [email protected], [email protected]
J. P. Blakeslee
Affiliation:
Dep. of Physics and Astronomy, Washington State University Pullman, WA 99164, USA email: [email protected], [email protected]
M. Capaccioli
Affiliation:
Dip. Scienze Fisiche, Univ. Federico II, I-80126, Napoli, Italy email: [email protected]
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Abstract

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Surface Brightness Fluctuations (SBF) are an useful distance indicator of gas-free galaxies as far as 100-150 Mpc with an accuracy of 5–10%. Recent applications have proved that the SBF technique is also a powerful tool to analyze the stellar content of elliptical-like galaxies by means of data/models comparison. Here we present a comprehensive study of the method on the base of a careful analysis of SBF models and a set of accurate multibands SBF measures obtained with HST.

Keywords

(galaxies:) Magellanic Cloudsgalaxies: evolutiongalaxies: stellar content
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 199 - 200
Copyright
Copyright © International Astronomical Union 2007

References

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