Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-26T03:04:39.535Z Has data issue: false hasContentIssue false
  • English
  • Français

Globular Clusters of the Inner Galactic Bulge

Published online by Cambridge University Press:  07 August 2017

Sergio Ortolani
Sergio Ortolani*
Affiliation:
Osservatorio Astronomico di Padova Vicolo dell'Osservatorio 5 35122 Padova Italy

Abstract

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.

Deep CCD photometry for a number of bulge-projected metal rich globular clusters and their nearby field background have been obtained. The V/V-I or I/V-I color-magnitude diagrams of the observed clusters are similar to the background fields and show high metallicity peculiar features. They are all very compact and slightly elongated.

Type
I. The Stellar Populations in the Milky Way
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 47 - 50
Copyright
Copyright © Kluwer 

References

Barbuy, B., Castro, S., Ortolani, S., Bica, E. 1991. A & A submitted.Google Scholar
Bressan, A., Bertelli, G., Chiosi, C. 1991. This volume.Google Scholar
Malkan, M. 1982, in Astrophysical Parameters for Globular Clusters , eds. Hayes, D.S., Philip, A.G.D., Davis Press, p. 533.Google Scholar
Ortolani, S., Barbuy, B., Bica, E. 1990. A & A, 236, 362.Google Scholar
Ortolani, S., Barbuy, B., Bica, E. 1991. A & A, in press.Google Scholar
Ortolani, S., Barbuy, B., Bica, E. 1991. A & A Letters, in press.Google Scholar
VandenBerg, D.A., Laskarides, P.G. 1987. Ap J Suppl., 64, 103.Google Scholar
Terndrup, D.M. 1988. A J, 96, 884.Google Scholar