Abstract
While the accuracy of photometric star counts rises, constraints on the
stellar population characteristics improve and allow synthetic models to be
conceived to explain the galactic structure. We show here how star counts have
significantly contributed to build a comprehensive picture of galactic evolution
and dynamics.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
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1. A Galactic structure primer;New Light on Dark Stars;2000
2. A Galactic structure primer;Springer Praxis Books