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The Present Data Situation for Stars in Open Clusters. II

Published online by Cambridge University Press:  14 August 2015

J.-C. Mermilliod
J.-C. Mermilliod*
Affiliation:
Institut d'Astronomie de l'Université de Lausanne et Observatoire de Genève

Extract

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The present state of astrometric, spectroscopic and photometric data for stars in 63 open clusters nearer to the Sun than 750 pc is summarized. Table I reports the limits of the available data in terms of the apparent V magnitude, in the same way as the previous version (Mermilliod 1977). Information on the apparent V magnitude of the brightest main sequence star (Vbr) and on the number of stars brighter than V=10 (n∗) has been included. In addition, the bluest spectral type on the main sequence has been used as an age estimator (TS).

Type
August 27 Introduction, Associations, Galactic Structure
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 129 - 133
Copyright
Copyright © Reidel 1980 

References

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