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UBV-Photometry and 35–day Cycle Model for X-ray Binary HZ Her/Her X–l

  • N. I. Shakura (a1), A. V. Smirnov (a1) and N. A. Ketsaris (a1)

Abstract

Based on the detailed analysis of UBV–photometry of HZ Her obtained in 1972–1994, a model of 35–day cycle is proposed in which both forced precession of a tilted accretion disk and free precession of the neutron star are present.

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References

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Gerend, D. & Boynton, P.E. 1976, ApJ, 209, 562
Howarth, I.D., & Wilson, R. 1983, MNRAS, 202, 347

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UBV-Photometry and 35–day Cycle Model for X-ray Binary HZ Her/Her X–l

  • N. I. Shakura (a1), A. V. Smirnov (a1) and N. A. Ketsaris (a1)

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