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2007 | 5 | 4 | 457-462
Tytuł artykułu

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

Treść / Zawartość
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
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.
Słowa kluczowe
Wydawca

Czasopismo
Rocznik
Tom
5
Numer
4
Strony
457-462
Opis fizyczny
Daty
wydano
2007-12-01
online
2007-12-01
Twórcy
  • Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám. 13, CZ-746 01, Opava, Czech Republic, terek@volny.cz
  • Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám. 13, CZ-746 01, Opava, Czech Republic
autor
  • Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám. 13, CZ-746 01, Opava, Czech Republic
Bibliografia
  • [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. http://dx.doi.org/10.1051/0004-6361:20030737[Crossref]
  • [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. http://dx.doi.org/10.1051/0004-6361:20010791[Crossref]
  • [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
  • [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. http://dx.doi.org/10.1051/0004-6361:20041377[Crossref]
  • [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.
  • [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. http://dx.doi.org/10.1002/asna.200510428[Crossref]
  • [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. http://dx.doi.org/10.1111/j.1365-2966.2007.11486.x[Crossref]
  • [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. http://dx.doi.org/10.1103/PhysRevLett.82.17[Crossref]
  • [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. http://dx.doi.org/10.1051/0004-6361:20047115[Crossref]
  • [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.
  • [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. http://dx.doi.org/10.1007/BF00756068[Crossref]
  • [13] M. Nowak and D. Lehr: “Theory of Black Hole Accretion Disks”, Cambridge University Press, Cambridge, 1999.
  • [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. http://dx.doi.org/10.1002/asna.200510417[Crossref]
  • [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. http://dx.doi.org/10.1111/j.1365-2966.2005.09214.x[Crossref]
  • [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. http://dx.doi.org/10.1111/j.1365-2966.2006.10571.x[Crossref]
  • [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. http://dx.doi.org/10.1086/311600[Crossref]
  • [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. http://dx.doi.org/10.1111/j.1365-2966.2006.11077.x[Crossref]
  • [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.
Typ dokumentu
Bibliografia
Identyfikatory
Identyfikator YADDA
bwmeta1.element.-psjd-doi-10_2478_s11534-007-0039-0
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