Hostname: page-component-669899f699-g7b4s Total loading time: 0 Render date: 2025-04-29T23:29:06.321Z Has data issue: false hasContentIssue false
  • English
  • Français

Non-Stability in Close Binary Stars

Published online by Cambridge University Press:  14 August 2015

V. A. Krat
V. A. Krat*
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.

Extract

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.

Those eclipsing binaries whose components are non-stable stars deserve particular attention not only owing to the fact that in such cases the physical properties of the stars may be studied in greater detail, but also since the mechanism of the ejection of gases from the atmospheres of the components may then be established with some certainty.

Type
V. Phenomena of Instability in Binary Systems
Information
Symposium - International Astronomical Union , Volume 3: Non-Stable Stars , 1957 , pp. 159 - 164
Copyright
Copyright © Cambridge University Press 1957 

References

1. Krat, V. A., Pulkovo Bull. 19, No. 2, 1 (1952).Google Scholar
2. Krat, V. A., Pulkovo Bull. 18, No. 4, 1 (1950).Google Scholar
3. Dadaev, A. N., Pulkovo Bull. 19, No. 5, 31 (1954).Google Scholar
4. Goldberg-Rogozinskaya, N. M., Pulkovo Bull. 18, No. 6, 64 (1951).Google Scholar
5. Sofronizky, A. V., Pulkovo Bull. 19, No. 4, 1 (1953).Google Scholar
6. Kuiper, G. P., Ap.J. 93, 133 (1941).Google Scholar
7. Mustel, E. R., Publ. Crim. Astrophys. Obs. 10, 143 (1953).Google Scholar