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Old LMC Globular Clusters: Reticulum

Published online by Cambridge University Press:  03 August 2017

Gianni Marconi ,
Vincenzo Ripepi ,
Gloria Andreuzzi ,
Giuseppe Bono ,
Roberto Buonanno  and
Santi Cassisi
Gianni Marconi
Affiliation:
ESO-Chile, Alonso de Cordova 3107 Casilla 19001, Santiago de Chile, Chile
Vincenzo Ripepi
Affiliation:
Naples Observatory, Via Moiarello 16, 80131 Napoli, Italy
Gloria Andreuzzi
Affiliation:
Rome Observatory, Via Frascati 33, 00040 Monte Porzio Catone, Italy
Giuseppe Bono
Affiliation:
Rome Observatory, Via Frascati 33, 00040 Monte Porzio Catone, Italy
Roberto Buonanno
Affiliation:
Rome Observatory, Via Frascati 33, 00040 Monte Porzio Catone, Italy
Santi Cassisi
Affiliation:
Teramo Observatory, Via M. Maggini, 64100 Teramo, Italy

Abstract

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We present a preliminary analysis of homogeneous, deep and accurate multiwavelength U, B, V, and I data of the old LMC cluster Reticulum. The comparison between theory and observations seems to suggest that the reddening toward this cluster is a factor of 2 larger than suggested in the literature. Both cluster distance and age are in agreement with the canonical values. Finally, the main goals of this project are briefly discussed.

Type
Part 1. The Star Clusters of Local Group Galaxies
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 193 - 195
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

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