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A composite color-magnitude diagram for a number of very poor clusterings in the Milky Way

Published online by Cambridge University Press:  04 August 2017

L.O. Lodén
L.O. Lodén*
Affiliation:
Astronomical Observatory, UPPSALA, Sweden

Extract

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There are indications of the presence of numerous stellar clusterings in the Milky Way which are so poor and unconspicuous that they become detected merely by accident. The true frequency of such objects is probably considerable as there is reason to believe that only a minor fraction has been detected.

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 117 - 118
Copyright
Copyright © Reidel 1984