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The circumstellar environments and variability of RY and RU Lup
Published online by Cambridge University Press: 04 August 2017
Abstract
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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