Abstract
The oscillations observed recently in the transient X-ray source A1118-61 are attributed to variations in the magnetic activity of a rotating white dwarf similar to the 11-year solar activity cycle. The transient nature, in analogy with the sun, is attributed to the variation in the strength of the cycle.
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Apparao, M. V. K. and Chitre, S. M.: 1970,Proc. Ind. Acad. Sci. 72A, 285,Proc. Int. Symp. on Pulsars and Supernovae, Rome (1972), pp. 291.
Böhm, K. H. and Cassinelli, D.: 1971,Astron. Astrophys. 12, 21.
Eyles, C. J., Skinner, G. K. and Willmore, A. P.: 1975,Nature 254, 577.
Ives, J. C., Sanford, P. W., and Bell Burnell, S. J.: 1975,Nature 254, 579.
Jones, C., Forman, W., and Liller, W.: 1973,Astrophys. J. 182, 109.
Kopecký, M.: 1963,Bull. Astr. Inst. Czechoslovakia 13, 340.
Pounds, K. A., Cooke, B. A., Ricketts, M. J., Turner, M. J., Peacock, A., and Eadie, G.: 1976,Astrophys. Space Sci. 42, 143.
Schatzman, E.: 1958,White Dwarfs, North-Holland Publishing Co., Amsterdam.
Wheaton, W. A., Baity, W. A., and Peterson, L. E.: 1975,IAU Circular No. 2761.
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Apparao, K.M.V., Chitre, S.M. Solar cycle model for oscillating transient X-ray sources. Astrophys Space Sci 42, 165–167 (1976). https://doi.org/10.1007/BF00645537
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DOI: https://doi.org/10.1007/BF00645537