Hostname: page-component-6bf8c574d5-9f2xs Total loading time: 0 Render date: 2025-03-09T17:10:02.090Z Has data issue: false hasContentIssue false
  • English
  • Français

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:

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Cohen, M., Schwartz, R.D.: 1976, Mon.Not.Roy.Astron.Soc. 174, 137.Google Scholar
Gahm, G.F.: 1978, Stockholm Obs. Report, No 14.Google Scholar
Gahm, G.F., Gehrsberg, R.E., Petrov, P.P., Shcherbakov, A.G., Kolotilov, E.A., Zaitseva, G.V., Shanin, G.I.: 1977, Variable Stars 20, 381.Google Scholar
Grinin, V.P., Efimov, Ju. S., Krasnobatsev, V.I., Shachovskaja, N.I., Shcherbakov, A.G., Zaitseva, G.V., Kolotilov, E.A., Shanin, G.I., Kiselev, N.N., Gjulaliev, Ch. G., Salmanov, I.R.: Variable Stars 21, 247.Google Scholar
Kholopov, P.N.: 1952, Variable Stars 9, 157.Google Scholar