Polarized emission from Black Hole Accretion Disks and Jets

APA

McKinney, J. (2014). Polarized emission from Black Hole Accretion Disks and Jets. Perimeter Institute for Theoretical Physics. https://pirsa.org/14110064

MLA

McKinney, Jonathan. Polarized emission from Black Hole Accretion Disks and Jets. Perimeter Institute for Theoretical Physics, Nov. 10, 2014, https://pirsa.org/14110064

BibTex

          @misc{ scivideos_PIRSA:14110064,
            doi = {10.48660/14110064},
            url = {https://pirsa.org/14110064},
            author = {McKinney, Jonathan},
            keywords = {Strong Gravity},
            language = {en},
            title = {Polarized emission from Black Hole Accretion Disks and Jets},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {nov},
            note = {PIRSA:14110064 see, \url{https://scivideos.org/pirsa/14110064}}
          }
          

Jonathan McKinney University of Maryland, College Park

Source Repository PIRSA
Collection

Abstract

We discuss how polarized emission can place constraints on the properties of accretion flows and jets in the strong gravity regime for systems like SgrA* and M87 being observed by the Event Horizon Telescope.