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Tomography of AM Her and QQ Vul

Published online by Cambridge University Press:  12 April 2016

A. Staude ,
A. D. Schwope ,
P. Hedelt ,
A. Rau  and
R. Schwarz
A. Staude
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
A. D. Schwope
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
P. Hedelt
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
A. Rau
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
R. Schwarz
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr. 11, 37083 Göttingen, Germany

Abstract

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We present optical high-resolution spectroscopy of AM Her and QQ Vul. Making use of indirect imaging techniques (Doppler and Roche tomography), we are able to make details visible, which a model of these systems has to be able to account for. Especially the emission line data cannot be explained by current models of polars.

Type
Part 5. Accretion Streams
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 251 - 257
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

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