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The Thick Disc Population of the Galaxy
Published online by Cambridge University Press: 07 August 2017
Extract
The availability of photometric and astrometric star counts on large fields well distributed in the Galaxy allows us to measure the characteristics of the thick disc population. We use a total of 19 data sets in UBV towards a dozen directions in order to measure the scale height, scale length, local density and metallicity of the intermediate population.
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- Copyright © Kluwer 1995