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V1016 Cyg: Proper Motion of Radio Emission

Published online by Cambridge University Press:  12 April 2016

S. P. S. Eyres ,
S. M. Dougherty ,
R. J. Davis ,
M. F. Bode ,
H. M. Lloyd  and
H. T. Kenny
S. P. S. Eyres
Affiliation:
University of Manchester, NRAL, Jodrell Bank, Macclesfield, Cheshire, SK11 9DL, UK
S. M. Dougherty
Affiliation:
Astrophysics Group, Liverpool John Moores University, Liverpool, L3 3AF, UK
R. J. Davis
Affiliation:
University of Manchester, NRAL, Jodrell Bank, Macclesfield, Cheshire, SK11 9DL, UK
M. F. Bode
Affiliation:
Astrophysics Group, Liverpool John Moores University, Liverpool, L3 3AF, UK
H. M. Lloyd
Affiliation:
Astrophysics Group, Liverpool John Moores University, Liverpool, L3 3AF, UK
H. T. Kenny
Affiliation:
Royal Military College, Kingston, Canada

Abstract

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We present MERLIN maps of V1016 Cyg at 6 cm, observed on 1992 July 21 and 1995 March 23. Previously discovered bipolar structure is resolved into three distinct peaks. Evolution and proper motion of these peaks has been measured.

Type
Novae & Symbiotic Stars
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 333 - 334
Copyright
Copyright © Kluwer 1996

References

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