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XMM observations of the long period polar V1309 Ori

Published online by Cambridge University Press:  12 April 2016

Robert Schwarz ,
Klaus Reinsch  and
Vadim Burwitz
Robert Schwarz
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
Klaus Reinsch
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
Vadim Burwitz
Affiliation:
Max-Planck Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany

Abstract

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We present the first full-orbit X-ray light curve of the remarkable eclipsing magnetic Cataclysmic Variable V1309 Ori obtained with XMM-Newton. The photometric behaviour and the extreme soft-to-hard flux ratio of the bright phase emission suggest that accretion occurs entirely via dense blobs.

Type
Part 5. Accretion Streams
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 276 - 277
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Beuermann, K. & Burwitz, V., 1995, ASP Conf. Ser. 85, 99 Google Scholar
Burwitz, V., Reinsch, K., Beuermann, K. & Thomas, H., 1999, ASP Conf. Ser. 157, 127 Google Scholar
Mauche, C. W., 1999, ASP Conf. Ser. 157, 157 Google Scholar
Staude, A., Schwope, A. D. & Schwarz, R., 2001, A&A 374, 588 Google Scholar