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Hybrid talk: Mega (6228, Hus 3, Albano) + https://stockholmuniversity.zoom.us/j/530682073
The puffy disk models have been constructed by us with a help of the GRRMHD Koral simulations. They share several aspects of thin, slim and thick accretion disks, but also differ from them considerably. They are magnetized, slightly sub-Eddington and thermally stable. They have interesting observational features that resemble some of the black hole sources.