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The Study of Stellar Populations and Dynamics in the Small Magellanic Cloud using the UKST

Published online by Cambridge University Press:  12 April 2016

D. Hatzidimitriou
D. Hatzidimitriou*
Affiliation:
Physics Department, University of Crete, GR 714-09 Heraklion, Crete, Greece

Abstract

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The combination of the wide field of Schmidt telescope photographic plates with fast measuring machines such as COSMOS and APM, had a major impact on the study of the global properties of the Magellanic Clouds. Results (based on UKST data) regarding the stellar populations and dynamics of the Small Magellanic Cloud are described here in some detail. The stellar content and kinematics of the intercloud region are also outlined, with particular emphasis on the importance of this region in understanding the interaction between the Magellanic Clouds.

Type
XI. Galaxies
Information
International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 396 - 404
Copyright
Copyright © Astronomical Society of the Pacific 1995

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