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The Variability of the T Tauri Star DI Cephei

Published online by Cambridge University Press:  12 April 2016

G.F. Gahm  and
P.P. Petrov
G.F. Gahm
Affiliation:
Stockholm Observatory, S-133 00 Saltsjöbaden, Sweden
P.P. Petrov
Affiliation:
Crimean Astrophysical Observatory, P/O Nauchny, Crimea, USSR

Abstract:

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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

References

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