Skip to main content
Log in

A remark about possible unity of the neutron star and black hole high frequency QPOs

  • Rapid Communication
  • Published:
Central European Journal of Physics

Abstract

In a series of papers it was discussed,on the basis of phenomenological arguments, whether the high frequency quasiperiodic oscillations (kHz QPOs)observed in the neutron-star and black-hole X-ray sources originate in the same physical mechanism. Recently it was suggested that a general trend seen in neutron star kHz QPOs instead excludes such a uniform origin. Using the example of the atoll source 4U 1636-53 we illustrate that this is not neccesarily true.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. W. Kluźniak and M.A. Abramowicz: “Strong-Field Gravity and Orbital Resonance in Black Holes and Neutron Stars — kHz Quasi-Periodic Oscillations (QPO)”, Phys. Rev. Lett. (submitted), 2000; see also Acta Phys. Pol. B Vol. 32 (2001), pp. 3605–3612.

  2. M.A. Abramowicz, T. Bulik, M. Bursa and W. Kluźniak: “Evidence for a 2:3 resonance in Sco X-1 kHz QPOs”, Astron. Astrophys., Vol. 404, (2003), p. L21.

    Article  ADS  Google Scholar 

  3. M.A. Abramowicz and W. Kluźniak: “A precise determination of black hole spin in GRO J1655-40”, Astron. Astrophys. Vol. 374, (2001), pp. L19–L20.

    Article  ADS  Google Scholar 

  4. J.E. McClintock and R.A. Remillard: “Black Hole Binaries”, In: Compact Stellar X-ray Sources, eds. W.H.G. Lewin and M. van der Klis, Cambridge University Press, Cambridge, 2005, Preprint arXiv:astro-ph/0306213

    Google Scholar 

  5. T. Belloni, M. Méndez and J. Homan: “The distribution of kHz QPO frequencies in bright low mass X-ray binaries”, Astron. Astrophys. Vol. 437, (2005), pp. 209–216.

    Article  ADS  Google Scholar 

  6. M.A. Abramowicz, D. Barret, M. Bursa, J. Horák, W. Kluźniak, P. Rebusco and G. Török: “A note on the slope-shift anticorrelation in the neutron star kHz QPOs data”, In: Proceedings of RAGtime 6/7, eds. S. Hledík and Z. Stuchlík, Silesian University in Opava, Opava, 2005, pp. 1–9.

    Google Scholar 

  7. M.A. Abramowicz, D. Barret, M. Bursa, J. Horák, W. Kluźniak, P. Rebusco and G. Török: “The correlations and anticorrelations in QPO data”, Astron. Nachr., Vol. 326, (2005), pp. 864–866.

    Article  ADS  Google Scholar 

  8. T. Belloni, M. Méndez and J. Homan: “On the kHz QPO frequency correlations in bright neutron star X-ray binaries”, Mon. Not. R. Astron. Soc., Vol.376, (2007), pp. 1133–1138.

    Article  ADS  Google Scholar 

  9. L. Stella and M. Vietri: “kHz Quasiperiodic Oscillations in Low-Mass X-Ray Binaries as Probes of General Relativity in the Strong-Field Regime”, Phys. Rev. Lett. Vol. 82, (1999), pp. 17–20.

    Article  ADS  Google Scholar 

  10. G. Török, M.A. Abramowicz, W. Kluźniak and Z. Stuchlík: “The orbital resonance model for twin peak kHz quasi periodic oscillations in microquasars”, Astron. Astrophys. Vol.436, (2005), pp. 1–8.

    Article  ADS  Google Scholar 

  11. M. Bursa: “High-frequency QPOs in GRO J1655-40: Constraints on resonance models by spectral fits”, In: Proceedings of RAGtime 6/7 eds. S. Hledík, Z. Stuchlík, Silesian University in Opava, Opava, 2005, pp. 39–45.

    Google Scholar 

  12. A.N. Aliev and D.V. Galtsov: “Radiation from Relativistic Particles in Nongeodesic Motion in a Strong Gravitational Field”, Gen. Relat. Gravit. Vol. 13, (1981), pp. 899–912.

    Article  ADS  MathSciNet  Google Scholar 

  13. M. Nowak and D. Lehr: “Theory of Black Hole Accretion Disks”, Cambridge University Press, Cambridge, 1999.

    Google Scholar 

  14. D. Barret, J.-F. Olive and M.C. Miller: “Drop of coherence of the lower kilo-Hz QPO in neutron stars. Is there a link with the innermost stable circular orbit?”, Astron. Nachr. Vol. 326, (2005), pp. 808–811.

    Article  ADS  Google Scholar 

  15. D. Barret, J.-F. Olive and M.C. Miller: “An abrupt drop in the coherence of the lower kHz quasi-periodic oscillations in 4U 1636-536”, Mon. Not. R. Astron. Soc. Vol. 361, (2005), pp. 855–860.

    Article  ADS  Google Scholar 

  16. D. Barret, J.-F. Olive and M.C. Miller: “The coherence of kilohertz quasi-periodic oscillations in the X-rays from accreting neutron stars”, Mon. Not. R. Astron. Soc. Vol. 370, (2006), pp. 1140–1146.

    Article  ADS  Google Scholar 

  17. M. Méndez, M. van der Klis, R. Wijnands, E.C. Ford, J. van Paradijs and B.A. Vaughan: “Kilohertz Quasi-periodic Oscillation Peak Separation Is Not Constant in the Atoll Source 4U 1608-52”, Astrophys. J., Vol. 505, (1998), p. L23.

    Article  ADS  Google Scholar 

  18. T. Belloni, J. Homan, S. Motta, E. Ratti and M. Mendez: “RossiXTE monitoring of 4U 1636-53:I. Long-term evolution and kHz Quasi-Periodic Oscillations”, Mon. Not. R. Astron. Soc., accepted,2007,Preprint arXiv:astro-ph/0705.0793.

  19. M.A. Abramowicz, P. Bakala, M. Bursa, J. Horák, W. Kluźniak, P. Rebusco, Z. Stuchlík and G. Török: in preparation, 2007

  20. M. Middleton, C. Done, M. Gierlinski and S.W. Davis: “Black hole spin in GRS 1915+105”, Mon. Not. R. Astron. Soc., Vol. 373, (2006), pp. 1004, Preprint arXiv:astro-ph/0601540.

    Article  ADS  Google Scholar 

  21. Z. Stuchlík, P. Bakala and G. Török: “On a multi-resonant origin of high frequency quasiperiodic oscillations in the neutron-star X-ray binary 4U 1636-53”, in preparation, 2007.

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Gabriel Török.

About this article

Cite this article

Török, G., Stuchlík, Z. & Bakala, P. A remark about possible unity of the neutron star and black hole high frequency QPOs. centr.eur.j.phys. 5, 457–462 (2007). https://doi.org/10.2478/s11534-007-0039-0

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.2478/s11534-007-0039-0

Keywords

PACS (2006)

Navigation