Abstract
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. © International Astronomical Union 2011.
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Tovmassian, G., Gänsicke, B., Zharikov, S., Ramirez, A., & Diaz, M. (2010). Do cataclysmic variables produce jets? In Proceedings of the International Astronomical Union (Vol. 6, pp. 311–312). Cambridge University Press. https://doi.org/10.1017/S174392131001625X
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