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On the Phases of Period Variation of SS 433

Published online by Cambridge University Press:  04 August 2017

W.Q. Luo
W.Q. Luo*
Affiliation:
Department of Physics, Sichuan Teachers' University, Chendu, Sichuan China

Extract

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In a previous paper (Luo, 1986), we have improved the method by Katz (1982) and Fan et al (1983). We have also found some important features in a ring model with precession and nodding motion, i.e., all the higher periodical components contain the ones with n = 1,2,3. So we can call T1,T2, and T3 fundamental periods.

Type
VI. Other Manifestations of Neutron Stars and Their Place in Neutron Star Evolution
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 551
Copyright
Copyright © Reidel 1987 

References

Fan, L.Z., and Li, S.X.: 1983, Scientia Sinica, No.5, 447.Google Scholar
Katz, J.I.: 1982, Astrophys. J., 260, 780.Google Scholar
Luo, W.Q.: 1986, Kue Xue Tongbao, 31, 523.Google Scholar
Newsom, G.H., and Collins, G.W.: 1982, preprint.Google Scholar
Mammano, A.: 1982, preprint.Google Scholar