No CrossRef data available.
Article contents
A Multicolor CCD Survey of Southern Globular Clusters
Published online by Cambridge University Press: 19 July 2016
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.
The existence of deviations of the observed photometric profiles with respect to the King models is a known fact (e.g., Newell and O'Neil, 1978; Aurière, 1983) and has been recently emphasized in the large survey by Kron et al., 1984. The origin of the light “excesses” (or defects) in the nuclear regions is, however, not very well understood. This work aims at clarifying this problem on the basis of multicolor (BVRIKC) CCD observations.
- Type
- Chapter X. Poster Papers on Formation and Evolution of Globular Clusters
- Information
- Copyright
- Copyright © Kluwer 1988
References
REFERENCES
Kron, G. E., Hewitt, A.V. and Wasserman, L. H.
1984
Publ. Astron. Soc. Pacific
96, 193.CrossRefGoogle Scholar
Webbink, R. F.
1985
1985 in
IAU Symposium No. 113. Dynamics of Star Clusters, Goodman, J. and Hut, P., eds., Reidel, Dordrecht, p. 541.Google Scholar