Emission From Point Sources In The Magellanic Clouds D.H. MORGAN, PASA, 15 (1), 123
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H
Emission From Point Sources In The Magellanic Clouds
D.H. MORGAN
ROYAL OBSERVATORY, BLACKFORD HILL, EDINBURGH, UK, EH9 3HJ
dhm@roe.ac.uk
Abstract:
Large numbers of the many types of emission-line object that are found in the Magellanic Clouds were first identified through H surveys of one kind or another. This paper looks at what has been achieved through such surveys and considers how the planned UKST H/TechPan Survey can further this kind of work.
Keywords: Magellanic Clouds, Stars - emission-line, Planetary Nebulae
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