Warm and thick corona for magnetically supported disk in GBHB

17 Sep 2019 Gronkiewicz Dominik Różańska Agata

This paper is devoted to self-consistent modeling of the magnetically supported accretion disk with optically thick warm corona based on first principles. In our model, we consider the gas heating by magneto-rotational instability (MRI) dynamo... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA