How Spatially Resolved Polarimetry Informs Black Hole Accretion Flow Models

Ricarte, Angelo; Johnson, Michael D.; Kovalev, Yuri Y.; Palumbo, Daniel C.M.; Emami, Razieh

doi:10.3390/galaxies11010005

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How Spatially Resolved Polarimetry Informs Black Hole Accretion Flow Models

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Kovalev, Yuri Y.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Ricarte, A., Johnson, M. D., Kovalev, Y. Y., Palumbo, D. C., & Emami, R. (2022). How Spatially Resolved Polarimetry Informs Black Hole Accretion Flow Models. Galaxies, 11(1), 5. doi:10.3390/galaxies11010005.

Cite as: https://hdl.handle.net/21.11116/0000-000C-CA4A-E

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