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Hyades Distance and Chemical Composition From the Competitive use of Astrometry, Photometry, Spectroscopy, and Internal Structure Computation

Published online by Cambridge University Press:  14 August 2015

G. Cayrel de Strobel
G. Cayrel de Strobel*
Affiliation:
Canada, France, Hawaii Telescope Corporation on leave of absence from Paris-Meudon Observatory

Abstract

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An analysis of observational astrometric, photometric, spectroscopic data for the Hyades cluster is performed in order to compare Hyades G dwarfs to the sun. Internal structure computations are also used to compare the solar ZAMS with the Hyades ZAMS and to discuss the constraints existing between distance and chemical composition for the cluster.

Type
August 27 Introduction, Associations, Galactic Structure
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 91 - 103
Copyright
Copyright © Reidel 1980 

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