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Physical Parameter Eclipse Mapping

Published online by Cambridge University Press:  12 April 2016

Sonja Vrielmann ,
Keith Horne ,
Raymundo Baptista  and
Frederick V. Hessman
Sonja Vrielmann
Affiliation:
School of Physics & Astronomy, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, Scotland, United Kingdom Universitäts-Sternwarte Göttingen, Geismarlandstr. 11, 37083 Göttingen, Germany
Keith Horne
Affiliation:
School of Physics & Astronomy, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, Scotland, United Kingdom
Raymundo Baptista
Affiliation:
Departamento de Fisica, Universidade Federal de Santa Catarina, Florianopolis, SC, 88040–900, Brazil
Frederick V. Hessman
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr. 11, 37083 Göttingen, Germany

Abstract

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We present a new eclipse mapping technique, which is able to map distributions in physical parameters of accretion disks in ecliping cataclysmic variables.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 820 - 821
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

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Vrielmann, S., Hessman, F.V., Horne, K. & Baptista, R. 1996, Proc. of the Keele Conf. on CVs, IAU Coll. 158, in pressGoogle Scholar