Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-25T15:44:17.409Z Has data issue: false hasContentIssue false
  • English
  • Français

Mapping the Line Emission Distribution of Cataclismic Variable Stars

Published online by Cambridge University Press:  12 April 2016

T.R. Marsh  and
K. Horne
T.R. Marsh
Affiliation:
Royal Greenwich Observatory, Hailshara, East Sussex, U.K.
K. Horne
Affiliation:
Space Telescope Science Institute, Baltimore, MD, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 85 - 89
Copyright
Copyright © Reidel 1987

References

Gull, S.F. & Skilling, J., 1984. in Indirect Imaging p267, ed. Roberts, J.A., Cambridge University Press Google Scholar
Horne, K.D., 1985. Mon. Not. R. astr. Soc. 213, 129 CrossRefGoogle Scholar
Horne, K.D. & Marsh, T.R., 1986. Mon. Not. R. astr. Soc. 218, 761 Google Scholar
Horne, K.D. & Steining, R.F., 1985. Mon. Not. R. astr. Soc. 216, 933 Google Scholar
Rowland, S.W., 1979. in Image reconstruction from projections p9, ed. Herman, G.T., Springer-Verlag Google Scholar
Skilling, J. & Bryan, R.K., 1984. Mon. Not. R. astr. Soc. 211, 111 Google Scholar
Smak, J., 1969. Acta Astron. 19, 155 Google Scholar