Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-27T05:12:20.883Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

REFERENCES

Gratton, R. 1985 Astron. Astrophys. 147, 169.Google Scholar
McClure, R. D., VandenBerg, D. A., Smith, G. H., Fahlman, G. G., Richer, B. B., Hesser, J. E., Harris, W. E., Stetson, P. B. and Bell, R. A. 1986 Astrophys. J. Letters 307, L49.CrossRefGoogle Scholar
Ratnatunga, K. V. and Bahcall, J. N. 1985 Astrophys. J. Suppl. 59, 63.CrossRefGoogle Scholar
VandenBerg, D. A. and Bell, R. A. 1985 Astrophys. J. Suppl. 58, 561.CrossRefGoogle Scholar
Sion, E. M. and Liebert, J. 1977 Astrophys. J. 213, 468.CrossRefGoogle Scholar