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The surface distribution clusters, planetary nebulae, supergiant M stars, and carbon stars in the Large Magellanic Cloud

Published online by Cambridge University Press:  14 August 2015

B. E. Westerlund
B. E. Westerlund*
Affiliation:
Mount Stromlo Observatory

Extract

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Some years ago the plates used for the extended Uppsala–Mount Stromlo Atlas of the Magellanic Clouds were searched for clusters in order to compare the optical extension of the Large Cloud with the one defined by the radio-astronomical observations of neutral hydrogen. Slightly over 150 clusters were identified and good agreement between the radio and optical boundaries was noted (Westerlund, unpublished data).

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 239 - 245
Copyright
Copyright © Australian Academy of Science 1964 

References

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