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UBV Photometry for 31 Galactic Globular Clusters
Published online by Cambridge University Press: 25 April 2016
Extract
For many reasons, it is important to have a sound body of reliable photometry for the globular clusters in the Milky Way galaxy. Given the striking appearance of the globular clusters and their historical and astrophysical interest, it is perhaps surprising that the available photoelectric photometry for globular clusters is of mixed quality (see Harris and Racine 1979). Here I present a homogeneous body of photometry through a single aperture and in the UBV system for 31 globular clusters south of declination +12°.
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- Copyright © Astronomical Society of Australia 1984