Facilitator: Ramesh Narayan, Harvard University
Air date: Tuesday, September 22, 2020
This session provides an introduction to the accretion phenomenon and family of hot accretion flow solutions within the broader framework of different accretion regimes.
Facilitator discusses relevant properties of hot flows: geometrically thick, optically thin, two-temperature, MAD/SANE magnetic fields, relativistic jets, uncertain thermodynamics, etc.
This session is part of a monthly series.
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