On the Hotspot Near a Kerr Black-Hole - Monte-Carlo Simulations

Details On the Hotspot Near a Kerr Black-Hole - Monte-Carlo Simulations On the Hotspot Near a Kerr Black-Hole - Monte-Carlo Simulations

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.269..283z&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 269, NO. 2/JUL15, P. 283, 1994

Physics

33

Scientific paper

The motion of a hotspot near a Kerr black hole is considered as a clear model of the variability of quasars and AGN. The evaluation of the model is based on Monte Carlo methods. The results are presented for equatorial circular motion of the hotspot. Key words: accretion, accretion discs - black hole physics - methods: statistical - galaxies: active - quasars: general.

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