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A wide field survey of Sagittarius dSph. Data and tools for the study of the Sgr Tidal Stream

Published online by Cambridge University Press:  01 December 2006

M. Correnti ,
M. Bellazzini ,
F. R. Ferraro  and
L. Monaco
M. Correnti
Affiliation:
Dipartimento di Astronomia, Universitá di Bologna, Italia email: matteo.correnti@studio.unibo.it
M. Bellazzini
Affiliation:
INAF – Osservatorio Astronomico di Bologna, Italia
F. R. Ferraro
Affiliation:
Dipartimento di Astronomia, Universitá di Bologna, Italia email: matteo.correnti@studio.unibo.it
L. Monaco
Affiliation:
European Southern Observatory, Santiago, Chile
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Abstract

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We present deep B,V,I photometry of three wide fields within the core of the Sagittarius dwarf spheroidal galaxy (Sgr dSph). We provide accurate templates for some well identified sequences of the CMD of the galaxy (Blue HB, Red HB, etc.) as tools to recognize portion of the tidal Stream detected by various surveys, to compare the stellar populations in the main body of Sgr and in its Stream, and to derive accurate distances to Stream stars.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 329 - 330
Copyright
Copyright © International Astronomical Union 2007

References

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