~105 M ☉ .25 kpc Run to z=0 Black Hole Physics: Environment-based seeding Seed mass 106 M ☉ Accretion Dynamical Friction Thermal Feedback Tremmel et al (2017) IASF - Milano 2019 Ray Sharma
dwarf galaxies, within a cosmological context. Isolated dwarf galaxies have diverse BH masses. Overmassive BH hosts have more rapid, earlier star formation than undermassive BH hosts. Overmassive BH hosts have lower central stellar density than undermassive BH hosts. Hosts of overmassive BHs can quench, maybe feedback? IASF - Milano 2019 Ray Sharma