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The circumstellar environments and variability of RY and RU Lup

Published online by Cambridge University Press:  04 August 2017

M. G. Hutchinson ,
A. Evans ,
J. Davies ,
M. Bode ,
D. Whittet  and
D. Kilkenny
M. G. Hutchinson
Affiliation:
1. Department of Physics, University of Keele
A. Evans
Affiliation:
1. Department of Physics, University of Keele
J. Davies
Affiliation:
2. Department of Space Research, University of Birmingham
M. Bode
Affiliation:
3. Department of Astronomy, Lancashire Polytechnic
D. Whittet
Affiliation:
3. Department of Astronomy, Lancashire Polytechnic
D. Kilkenny
Affiliation:
4. South African Astronomical Observatory

Abstract

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The variability of the two T Tauri stars RY and RU Lup has been monitored between 1980 and 1984 at both optical and infrared wavelengths. We present here a preliminary analysis of the data and suggest possible mechanisms for the observed variability.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 109 - 112
Copyright
Copyright © Reidel 1987 

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