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Two-Frequency VLA Monitoring of LSI+61°303 during a Full Radio Period

Published online by Cambridge University Press:  12 April 2016

J. M. Paredes ,
M. Peracaula ,
M. Ribó ,
J. Martí ,
M. Tavani ,
D. A. Kniffen  and
J. R. Mattox
J. M. Paredes
Affiliation:
Departament d’Astronomia i Meteorologia, Universitat de Barcelona, Barcelona, Spain
M. Peracaula
Affiliation:
Departament d’Astronomia i Meteorologia, Universitat de Barcelona, Barcelona, Spain
M. Ribó
Affiliation:
Departament d’Astronomia i Meteorologia, Universitat de Barcelona, Barcelona, Spain
J. Martí
Affiliation:
CEA / DSM / DAPNIA / Service d’Astrophysique, Centre d’Études de Saclay, F-91191 Gif-Sur-Yvette, France
M. Tavani
Affiliation:
Columbia Astrophysics Laboratory, Columbia University, New York, NY, U.S.A.
D. A. Kniffen
Affiliation:
Department of Physics and Astronomy, Hampden-Sydney College, VA, U.S.A.
J. R. Mattox
Affiliation:
Astronomy Department, Boston University, Boston, MA, U.S.A.

Abstract

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We report observations of the radio periodic Be X-ray binary LSI+61°303, obtained with the VLA at 3.6 and 2.0 cm during a full 26.5 d cycle. These observations were carried out in coordination with CGRO monitoring of its possible γ-ray counterpart 2CG 135+1.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 347 - 348
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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