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The Variability of the T Tauri Star DI Cephei
Published online by Cambridge University Press: 12 April 2016
Abstract:
It is demonstrated that the light variations of DI Cephei can be explained as due to the combined effect of variable completely grey circumstellar extinction and variable continuous and line emission.
- Type
- Session III: Observed Activity in Related Objects
- Information
- International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 497 - 500
- Copyright
- Copyright © Reidel 1983