No CrossRef data available.
Article contents
The Galactic Distance Scale: Globular Clusters
Published online by Cambridge University Press: 14 August 2015
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.
A new compilation of distance data for the Galactic globular clusters is used to estimate the distance to the Galactic center, RO. Three different ways of using the space distribution of the clusters lead to RO = (8.5 ± 1.0) kpc. The problem of the space distribution of the clusters in the Galactic nuclear region is briefly discussed.
- Type
- August 27 Introduction, Associations, Galactic Structure
- Information
- Copyright
- Copyright © Reidel 1980
References
Arp, H.C.: 1965, in “Galactic Structure”, ed. Blaauw, A. and Schmidt, M. (Chicago: U. Chicago Press), p.401.Google Scholar
Baade, W.: 1958, in “Stellar Populations”, ed. O'Connell, D.J.K. (New York: Interscience), p.303.Google Scholar
Demarque, P., and McClure, R.D.: 1977, in “Evolution of Galaxies and Stellar Populations”, ed. Tinsley, B.M. and Larson, R.B. (New Haven: Yale U. Obs.), p.199.Google Scholar