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Hα Emission from Point Sources in the Magellanic Clouds

Published online by Cambridge University Press:  16 May 2016

D. H. Morgan
D. H. Morgan*
Affiliation:
Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK; dhm@roe.ac.uk
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Abstract

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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.

Keywords

Magellanic Cloudsstars: emission-lineplanetary nebulae
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 15 , Issue 1 , 1998 , pp. 123 - 127
Copyright
Copyright © Astronomical Society of Australia 1998

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