Two-temperature magnetically arrested disk simulations with turbulent electron heating are resolution-converged and produce emission similar to the simpler R(beta) parametric model, with a moderate spin of a*=0.5 matching Sgr A* ALMA data best.
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Revision of two-temperature magnetically arrested flows onto a black hole
Two-temperature magnetically arrested disk simulations with turbulent electron heating are resolution-converged and produce emission similar to the simpler R(beta) parametric model, with a moderate spin of a*=0.5 matching Sgr A* ALMA data best.