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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.

Information

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