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RS Ophiuchi - A Recurrent Nova with Twin Jets

Published online by Cambridge University Press:  03 August 2017

R. J. Davis ,
A. R. Taylor ,
M. F. Bode  and
R. W. Porcas
R. J. Davis
Affiliation:
NRAL, Jodrell Bank
A. R. Taylor
Affiliation:
NRAL, Jodrell Bank
M. F. Bode
Affiliation:
Lancashire Polytechnic
R. W. Porcas
Affiliation:
MPI Bonn

Abstract

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An analysis of European VLBI data of nova RS Ophiuchi shows the presence of a linear jet-like structure which has a brightness temperature of 107K at 1.7 GHz. This ejection is shown to be two sided and the 1.7 GHz emission is non-thermal. The light curves show the presence of a second, thermal component emerging at higher frequencies at a later epoch.

Type
Galactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 277 - 278
Copyright
Copyright © Reidel 1988 

References

Hjellming, R.M., van Gorkom, J.J., Taylor, A.R., Seaquist, E.R., Padin, S., Davis, R.J. & Bode, M.F. (1986). Ap. J. Lett. 305, L71–L75.CrossRefGoogle Scholar
Morrison, W. (1985). IAU Circ. No. 4030.Google Scholar
Padin, S., Davis, R.J. & Bode, M.F., (1985). Nature, 315, 306 CrossRefGoogle Scholar