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Attempt to Apply the U B V B1B2V1G Photometry to the Determination of the Distance of the Hyades

Published online by Cambridge University Press:  07 February 2017

M. Golay*
Affiliation:
Observatoire de Genève, Switzerland

Abstract

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A photometric method, using the U B V B1B2V1G system, is suggested to determine the distance of clusters. This method based on the assumption that stars with same seven colours have also same absolute visual magnitude is applied, as an example, to Hyades and Praesepe.

Type
Part II: Absolute Magnitudes from Galactic Clusters and Associations
Copyright
Copyright © Reidel 1973 

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