Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-04-30
Astronomy and Astrophysics
Astrophysics
15 pages, 4 figures, AASTeX. Accepted for publication in Astrophysical Journal Letters
Scientific paper
We report the discovery with the proportional counter array (PCA) onboard the Rossi X-ray Timing Explorer (RXTE) of a 450 Hz quasiperiodic oscillation (QPO) in the hard X-ray flux from the galactic microquasar GRO J1655-40. This is the highest frequency QPO modulation seen to date from a black hole. The QPO is detected only in the hard X-ray band above 13 keV. It is both strong and narrow, with a typical rms amplitude of 4.5 % in the 13 - 27 keV range, and a width of 40 Hz (FWHM). For two observations in which we detect the 450 Hz QPO a previously known 300 Hz QPO is also observed in the 2 - 13 keV band. We show that these two QPO sometimes appear simultaneously, thus demonstrating the first detection of a pair of high frequency QPO in a black hole system. Prior to this, pairs of high frequency QPO have only been detected in neutron star systems. GRO J1655-40 is one of only a handful of black hole systems with a good dynamical mass constraint. For a non-rotating black hole with mass between 5.5 - 7.9 solar masses, the innermost stable circular orbit (ISCO) ranges from 45 - 70 km. For any mass in this range the radius at which the orbital frequency reaches 450 Hz is less than the ISCO radius, indicating that if the modulation is caused by Kepler motion, the black hole must have appreciable spin. If the QPO frequency is set by the orbital frequency of matter at the ISCO then for this mass range the dimensionless angular momentum lies between 0.15 < j < 0.5. Moreover, if the modulation is caused by oscillation modes in the disk or Lense-Thirring precession, then this would also require a rapidly rotating hole. We briefly discuss the implications of our findings for models of X-ray variability in black holes and neutron stars.
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