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Physical Parameter Mapping of Accretion Disks

Published online by Cambridge University Press:  12 April 2016

S. Vrielmann ,
F. V. Hessman ,
K. Horne  and
R. Baptista
S. Vrielmann
Affiliation:
Universitäts-Sternwarte Göttingen, Germany
F. V. Hessman
Affiliation:
Universitäts-Sternwarte Göttingen, Germany
K. Horne
Affiliation:
University of St. Andrews, Scotland, UK
R. Baptista
Affiliation:
University of St. Andrews, Scotland, UK

Abstract

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We present a further development of the classical eclipse mapping method, which reconstructs the spatial distribution of physical parameters in the accretion disks of cataclysmic variables.

Type
Accretion Discs
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 125 - 126
Copyright
Copyright © Kluwer 1996

References

Baptista, R., Steiner, J.E., 1991, A&A,, 249, 284 Google Scholar
Baptista, R., Horne, K., Hilditch, R.W., et al., 1995, Ap. J., 448, 395 Google Scholar
Horne, K., 1985, MNRAS, 213, 129 Google Scholar
Horne, K., 1995, A&A, 297, 273 Google Scholar
Horne, K., Marsh, T.R., 1986, MNRAS, 218, 761 Google Scholar
Skilling, J., Bryan, R.K., 1984, MNRAS, 211, 111 CrossRefGoogle Scholar
Wood, J.H., Horne, K., Vennes, S., 1992, Ap. J., 385, 294 Google Scholar