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Hα Emission from Point Sources in the Magellanic Clouds
Published online by Cambridge University Press: 16 May 2016
Abstract
Large numbers of the many types of emission-line object that are found in the Magellanic Clouds were first identified through Hα surveys of one kind or another. This paper looks at what has been achieved through such surveys and considers how the planned UKST Hα/TechPan Survey can further this kind of work.
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- Research Article
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- Copyright © Astronomical Society of Australia 1998
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