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Variations of VLBI Structure in UX Ari

Published online by Cambridge University Press:  03 August 2017

M. Catarzi ,
M. Felli ,
M. Massi ,
F. Palagi ,
R. Pallavicini  and
G. Tofani
M. Catarzi
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy
M. Felli
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy
M. Massi
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy
F. Palagi
Affiliation:
Gruppo Nazionale di Astronomia, CNR, Largo E. Fermi 5, 50125 Florence, Italy
R. Pallavicini
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy
G. Tofani
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy

Extract

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Five stellar binary systems of RS CVn and Algol type have been observed on June 12, 1986, with the EVN (Effelsberg, Jodrell, Medicina, Onsala, Westerbork), and two US antennas (Green Bank, Haystack). Observations were carried out at 5 GHz, with 13 min of integration and with MARK III mode B.

Type
Galactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 283 - 284
Copyright
Copyright © Reidel 1988 

References

Mutel, R.L., Lestrade, J.F., Prenston, R. A. and Phillips, R.B.: 1985, Ap. J. 298, 262.Google Scholar