Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-12-04T19:49:23.808Z Has data issue: false hasContentIssue false
  • English
  • Français

Core and Tidal Radii of the Carina Dwarf Spheroidal Galaxy from UK Schmidt Telescope Plates

Published online by Cambridge University Press:  04 August 2017

P. J. Godwin
P. J. Godwin*
Affiliation:
Department of Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, Scotland, U.K.

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.

Core and tidal radii of the Carina dwarf galaxy are determined by fitting King dynamical models to number count radial profiles, derived from COSMOS data. These values are compared with those of the other six known Local Group dwarf spheroidals.

Type
May 29: Observations of Globular Clusters
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985 , pp. 77 - 79
Copyright
Copyright © Reidel 1985 

References

Godwin, P.J. (1984) PhD Thesis, University of Edinburgh (in prep.) Google Scholar
Hodge, P.W., Michie, R.W. (1969) Astron. J. 74 p587 Google Scholar
King, I.R. (1962) Astron. J. 67 p471 Google Scholar
King, I.R. (1965) Astron. J. 70 p376 Google Scholar
King, I.R. (1966) Astron. J 71 p64 CrossRefGoogle Scholar
Mould, J.R., Aaronson, M. (1983) Ap. J. 273 p530.Google Scholar