The S-shaped limit cycle of accretion disk and quasi-periodic variation of BL Lac object ON231

Statistics – Computation

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Accretion Disks, Bl Lacertae Objects, Black Holes (Astronomy), Computational Astrophysics, Dwarf Novae, Luminosity

Scientific paper

The observed outburst behavior of ON + 231 is analyzed with reference to theoretical models. The approach applied is based on: (1) the dwarf-nova model of Meyer and Meyer-Hofmeister (1981 and 1982), involving thermal instability related to the peak in the opacity curve at temperatures where hydrogen is partially ionized; and (2) the model of Lin and Shields (1986) for the long-period outbursts of AGN and Seyferts. For the BL Lac-type supermassive black hole in a thin disk, an S-shaped limit-cycle curve is obtained which accounts for the quasi-periodic outbursts of ON + 231.

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