Probing the Magnetic Field Structure in Sgr A* on Black Hole Horizon Scales with Polarized Radiative Transfer Simulations

Probing the Magnetic Field Structure in Sgr A* on Black Hole Horizon Scales with Polarized Radiative Transfer Simulations

Magnetic fields are believed to drive accretion and relativistic jets in black hole accretion systems, but the magnetic field structure that controls these phenomena remains uncertain. We perform general relativistic (GR) polarized radiative transfer of time-dependent three-dimensional GR magnetohyd...

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Bibliographic Details
Main Authors: Gold, Roman, McKinney, Jonathan C., Johnson, Michael D., Doeleman, Sheperd Samuel
Other Authors: Haystack Observatory
Format: Article
Language:en_US
Published: IOP Publishing 2017
Online Access:http://hdl.handle.net/1721.1/110005

Internet

http://hdl.handle.net/1721.1/110005

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