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Deep CCD Photometry in ω Cen and NGC 3201+

Published online by Cambridge University Press:  19 July 2016

S. Ortolani
S. Ortolani*
Affiliation:
Asiago Astrophysical Observatory

Extract

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About 30 deep B and V CCD images, obtained at the 3.6 m ESO telescope, with the EFOSC in the focal reducer option, have been used to obtain color-magnitude diagrams and luminosity functions for the main sequence of the globular clusters ω Cen and NGC 3201. Two fields per cluster, at different distances from the center (25′ − 30′ for ω Cen and 7′.5 − 9′ for NGC 3201) were observed and separately reduced.

Type
Chapter IX. Poster Papers on Cluster Systems in Distant Galaxies. Deep Photometry and CM Diagrams
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 629 - 630
Copyright
Copyright © Kluwer 1988 

References

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