Strong-field gravity and orbital resonance in black holes and neutron stars -khz quasi-periodic oscillations (QPO)

Acta Physica Polonica B

Volumn 32, Issue 11, 2001, Pages 3605-3612

  Kluzniak, Wlodek ^a,c   Abramowicz, Marek Artur ^b,d  

^a UNIVERSITY OF ZIELONA GÓRA   (Poland)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^c NORDITA   (Denmark)

^d CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 31244435927     PISSN: 05874254     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Article

References (7)

1. M. van der Klis, Annu. Rev. Astron. Astrophys. 38, 717 (2000).
2. It is thought that fluid in accretion disks of small vertical extent ("thin disks") approximately follows circular geodesic trajectories. Observations of water masers in some thin disks in active galactic nuclei (AGNs) do indeed reveal a Keplerian distribution of velocity for the water masers, v = fir = (GM/r)1/2: M. Miyoshi, et al, Nature 373, 127 (1995).
3. S. Kato, S. Mineshige, J. Fukue, Black Hole Accretion Disks, Kyoto University Press, Kyoto 1998.
4. [4j S. Kato, J. Fukue, Proc. Astron. Soc. Japan, 32, 377 (1980).
5. L.D. Landau, E.M. Lifschitz, Classical Mechanics, Pergamon, 1973.
6. T.E. Strohmayer, Astrophys. J. 552, L49 (2001).
7. M.A. Abramowicz, W. Kluzniak, Astron. Astrophys. 374, L19 (2001).