A Toy Model for 3:2 Ratio of kHz QPO Frequency in Black Hole X-ray Binaries

Details A Toy Model for 3:2 Ratio of kHz QPO Frequency in Black Hole X-ray Binaries A Toy Model for 3:2 Ratio of kHz QPO Frequency in Black Hole X-ray Binaries

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005chjas...5....7w&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 5 Supplement, p. 7-12

Physics

Accretion, Accretion Disks, Black Hole Physics, X-Rays: Stars, Microquasars

Scientific paper

Production of pairs of high frequency quasi-periodic oscillations (QPOs) in black hole X-ray binaries is discussed based on a model of non-axisymmetric magnetic coupling of a rotating black hole (BH) with its surrounding accretion disk, in which a puzzling 3:2 ratio of the upper frequency to the lower frequency is explained. In addition, the correlation of the pairs of high frequency QPOs with the jets from microquasars is discussed.

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