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Mapping the Line Emission Distribution of Cataclismic Variable Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
We describe a method for imaging the accretion disc of a Cataclysmic Variable star. We use the two-dimensional information contained in the line profiles as they vary with phase to invert the line formation process. Asymmetries in the disc, as are caused by the bright-spot, for example, are accounted for naturally.
- Type
- II. Radio, IR and Optical Observations
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- Copyright
- Copyright © Reidel 1987