• CGCA Seminar – Daniel Palumbo

    Kenwood IRC 2175 Milwaukee, WI, United States

    Spin Signatures in Horizon-Resolved Images of LLAGN
    Dr. Daniel Palumbo, Smithsonian Astrophysical Observatory
    Harvard University

    With the advent of the Event Horizon Telescope (EHT), near-horizon black hole imaging with sub-mm very-long-baseline interferometry (VLBI) is now routine for the two sources for which terrestrial VLBI is sufficient to resolve the black hole shadow: Messier 87* and Sagittarius A*. Since the first images of M87*, the theoretical analysis of these images has advanced a broad class of black hole spin tracers in horizon-resolving observations, all of which have complex interplay with the astrophysical conditions near the horizon. Meanwhile, space VLBI mission concepts such as the Black Hole Explorer aim to drastically improve the angular resolution available via sub-mm VLBI, resolving out the primary accretion disk image to isolate the strongly lensed "photon ring," which more robustly exposes black hole mass, spin, and viewing inclination to distant observers.

  • CGCA Seminar – Joaquin Duran

    Kenwood IRC 2175 Milwaukee, WI, United States

    A Parameter Study of Eccentric Accretion Disks in GRMHD
    Joaquin Duran
    University of Texas at San Antonio

    We present a three dimensional GRMHD parameter study of circularized and eccentric black hole accretion disks using the KORAL code. Our simulations span SANE and MAD magnetic flux states, black hole spins of a=0 and a=0.9, and disk eccentricities of e=0, 0.38, and 0.5. We investigate how orbital eccentricity changes disk morphology, radial inflow, magnetization, accretion variability, outflow efficiency, and disk outflow orientation. Eccentric disks develop stronger nonaxisymmetric structure and shock heated spiral features, while their radial inflow differs from circularized controls. The magnetic response depends strongly on flux state: eccentric SANE models are less magnetized and less variable, while eccentric MAD models are more magnetized and more variable. In MAD, eccentricity is also associated with larger disk and magnetized polar outflow orientation excursions.

  • CGCA Seminar – Nick Conroy

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Nick Conroy
    IAA/CfA

    The abstract for this talk will be added as soon as it is made available.

  • CGCA Seminar – Patrick Brady

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Patrick Brady
    Professor, University of Wisconsin-Milwaukee

    The abstract for this talk will be added as soon as it is made available.

  • CGCA Seminar – Alexander W. Criswell

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Alexander W. Criswell
    Vanderbilt University

    The abstract for this talk will be added as soon as it is made available.

  • CGCA Seminar – Pratyasha Gitika

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Pratyasha Gitika
    Postdoctoral Scholar, University of Wisconsin-Milwaukee

    The abstract for this talk will be added as soon as it is made available.

  • CGCA Seminar – Matthew Todd

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Matthew Todd
    Postdoctoral Scholar, MIT

    The abstract for this talk will be added as soon as it is made available.

  • CGCA Seminar – Vedant Dhruv

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Vedant Dhruv
    Postdoctoral Scholar, Washington University St. Louis

    The abstract for this talk will be added as soon as it is made available.