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Double radio peak and non-thermal collimated ejecta in RS Ophiuchi following the 2006 outburst
Authors:S. P. S. Eyres,T. J. O'Brien,R. Beswick,T. W. B. Muxlow,G. C. Anupama,N. G. Kantharia,M. F. Bode,M. P. Gawro&#  ski,R. Feiler,A. Evans,M. T. Rushton,R. J. Davis,T. Prabhu,R. Porcas, B. J. M. Hassall
Affiliation:Jeremiah Horrocks Institute for Astrophysics and Supercomputing, University of Central Lancashire, Preston PR1 2HE;Jodrell Bank Centre for Astrophysics, The Alan Turing Building, The University of Manchester, Manchester M13 9PL;Indian Institute of Astrophysics, II Block Koramangala, Bangalore 560 034, India;National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune University Campus, Post Bag 3, Ganeshkind, Pune 411007, India;Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD;ToruńCentre for Astronomy, Nicolas Copernicus University, ul. Gagarina 11, 87–100 Toruń, Poland;Astrophysics Group, Keele University, Keele, Staffordshire ST5 5BG;Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D–53121 Bonn, Germany
Abstract:
Keywords:stars: individual: RS Oph    novae, cataclysmic variables    stars: winds, outflows    radio continuum: stars
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