www.vikrammanikantan.com
we use GRMHD simulations and radiative transfer to show that eccentric binary black holes are unique in their accretion rate, jet power, and synchrotron emission in IR and optical wavelengths
we use GRMHD simulations and radiative transfer to show that eccentric binary black holes are unique in their accretion rate, jet power, and synchrotron emission in IR and optical wavelengths