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23. Evidence for and against the binary nature of some Tio-he II-nebular variables, and the possible amplification of B-star eruptions by a cool companion

Published online by Cambridge University Press:  02 August 2017

Martin Johnson

Extract

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1. This problem might be deprecated as requiring for its solution more evidence than now exists; but, even though it cannot yet be conclusively solved, it will introduce some consideration of possible interactions between binary components and between different atmospheric regions of a single star, which may help to explain other peculiar variable spectra.

Type
Part IV Symposia
Information
Transactions of the International Astronomical Union , Volume 8 , September 1954 , pp. 839 - 842
Copyright
Copyright © Cambridge University Press 1954

References

(1) Swings, and Struve, : Series on Peculiar Stars in Ap. J 91–98, 1940–3.Google Scholar
(2) Merrill, : Ap. J. 81, 312, 1935; 99 , 15, 1944; III, 484, 1950.Google Scholar
(3) Payne-Gaposchkin, C.: Ap. J 104, 357 and 362, 1946.Google Scholar
(4) Struve, : Rev. Mod. Physics, 16, 293, 1944.Google Scholar
(5) Merrill, : Ap. J 112, 514, 1950.Google Scholar
(6) Johnson, M.: M.N. 111, 490, 1951.Google Scholar
(7) Joy, : AP. J 106, 288, 1947.Google Scholar
(8) Gaposchkin, S. and Gaposchkin, C. P.: Variable Stars, p. 301, 1938.Google Scholar
(9) Struve, : Stellar Evolution, p. 193, 1950.Google Scholar
(10) Baldwin, R. B.: Ap. J 92, 82, 1940.Google Scholar
(11) Kuiper, G. P: Ap. J 93, 133, 1941.Google Scholar
(12) Hoyle, and Lyttleton, : M.N. 103, 22, 1943.Google Scholar
(13) Biermann, L.: Z. Astrophysik, 18, 344, 1939.Google Scholar
(14) Gerasimovic, : M.N. 94, 737, 1934.Google Scholar
(15) Underhill, A. B.: M.N. 109, 562, 1949.Google Scholar