Halpha Emission from Point Sources in the Magellanic Clouds
DH Morgan
Publications of the Astronomical Society of Australia
15(1) 123 - 127
Published: 1998
Abstract
Large numbers of the many types of emission-line object that are found in the Magellanic Clouds were first identified through Halpha surveys of one kind or another. This paper looks at what has been achieved through such surveys and considers how the planned UKST Halpha/TechPan Survey can further this kind of work.https://doi.org/10.1071/AS98123
© ASA 1998
