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Core and Tidal Radii of the Carina Dwarf Spheroidal Galaxy from UK Schmidt Telescope Plates
Published online by Cambridge University Press: 04 August 2017
Abstract
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