Quasi-Periodic Features Due to Clumps Orbiting around a Black Hole

Details Quasi-Periodic Features Due to Clumps Orbiting around a Black Hole Quasi-Periodic Features Due to Clumps Orbiting around a Black Hole

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pasj...51..317k&link_type=abstract

Publications of the Astronomical Society of Japan, v.51, p.317-320.

Astronomy and Astrophysics

Astronomy

13

Accretion Disks, Black Holes, X-Rays: Sources

Scientific paper

The expected Fourier power-spectrum density is examined with regard to the shape and quality factor Q of features which are predicted to appear in a signal from clumps orbiting near a marginally stable orbit of a compact body. It is shown that clumps distributed randomly in a narrow range of radii produce quasi-periodic oscillations with Q~102, similar to those observed in many low-mass X-ray binaries.

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