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

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.

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Item Permalink: https://hdl.handle.net/21.11116/0000-000C-CA4A-E Version Permalink: https://hdl.handle.net/21.11116/0000-000C-CA4B-D

Genre: Journal Article

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Ricarte, Angelo, Author
Johnson, Michael D., Author
Kovalev, Yuri Y.¹, Author
Palumbo, Daniel C.M., Author
Emami, Razieh, Author

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1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: Astrophysics - High Energy Astrophysical Phenomena

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Dates: Date issued: 2022-12

Publication Status: Issued

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Identifiers: DOI: 10.3390/galaxies11010005
BibTex Citekey: 2022Galax..11....5R

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Title: Galaxies

Source Genre: Journal

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Pages: - Volume / Issue: 11 (1) Sequence Number: - Start / End Page: 5 Identifier: -