Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-25T05:10:05.876Z Has data issue: false hasContentIssue false

The Spatial Distribution of Young Objects in the Large Magellanic Cloud - A Problem of Pattern Recognition

Published online by Cambridge University Press:  04 August 2017

J. V. Feitzinger
Affiliation:
Astronomisches Institut der Ruhr-Universität, Bochum, BRD
E. Braunsfurth
Affiliation:
Astronomisches Institut der Ruhr-Universität, Bochum, BRD

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.

Methods used in pattern recognition and cluster analysis are applied to investigate the spatial distribution of OB associations and emission regions in the LMC. For our analysis we used the catalogue of associations of Lucke and Hodge (1970) and the catalogue of emission regions of Davies et al. (1976).

Type
Evolution
Copyright
Copyright © Reidel 1984 

References

Anderberg, M.R., 1973, Cluster Analysis for Applicants, Academic Press, New York Google Scholar
Davies, R.D., Elliott, K.H., Meaburn, J., 1976, Mem. Roy. Astr. Soc. 81, 89 Google Scholar
Feitzinger, J.V., 1980, Space Science Rev. 27, 35 Google Scholar
Lucke, P.B., Hodge, P.W., 1970, Astron. J. 75, 171 CrossRefGoogle Scholar
Martin, N., Prevot, L., Rebeirot, E., Rousseau, J., 1976, Astron. Astrophys. 51, 31 Google Scholar
Meaburn, J., 1980, MN 192, 365 Google Scholar
Meaburn, J., 1981, in: Investigating the Universe, ed. by Kahn, F.D., Reidel Pub. Comp., Dordrecht, p. 61 Google Scholar
Schmidt-Kaler, Th., 1977, Astron. Astrophys. 54, 771 Google Scholar