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Do cataclysmic variables produce jets?

Published online by Cambridge University Press:  24 February 2011

G. Tovmassian ,
B. Gänsicke ,
S. Zharikov ,
A. Ramirez  and
M. Diaz
G. Tovmassian
Affiliation:
Instituto de Astronomía, UNAM, México
B. Gänsicke
Affiliation:
Dept of Physics, University of Warwick, UK
S. Zharikov
Affiliation:
Instituto de Astronomía, UNAM, México
A. Ramirez
Affiliation:
Instituto de Astronomía, UNAM, México
M. Diaz
Affiliation:
IAGCA, Universidade de São Paulo, Brazil
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Abstract

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It is believed that CVs do not produce jets unlike other, more massive interactive binaries. Here we present spectrophotometric observations of the super-outburst of V455 And. We show here that a strong wind perpendicular the the accretion disc at the maximum of the super-otburst, i.e a jet, can probably explain the observed spectroscopic behavior of this system.

Keywords

(stars:) binaries: spectroscopic(stars:) novaecataclysmic variables
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S275: Jets at all Scales , September 2010 , pp. 311 - 312
Copyright
Copyright © International Astronomical Union 2011

References

Ribeiro, F. M. A. & Diaz, M. P. 2008, PASJ, 60, 327CrossRefGoogle Scholar
Araujo-Betancor, et al. , 2005, A&A, 430, 629Google Scholar