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A chemical model for the interstellar medium in galaxies
Stefano Bovino, Tommaso Grassi, Pedro R. Capelo +2
We present and test chemical models for three-dimensional hydrodynamical simulations of galaxies. We explore the effect of changing key parameters such as metallicity, radiation an…
A comparison of black hole growth in galaxy mergers with Gasoline and Ramses
J. M. Gabor, Pedro R. Capelo, Marta Volonteri +4
Supermassive black hole dynamics during galaxy mergers is crucial in determining the rate of black hole mergers and cosmic black hole growth. As simulations achieve higher resoluti…
Growing black holes and galaxies: black hole accretion versus star formation rate
Marta Volonteri, Pedro R. Capelo, Hagai Netzer +3
We present a new suite of hydrodynamical simulations and use it to study, in detail, black hole and galaxy properties. The high time, spatial and mass resolution, and realistic orb…
Black hole accretion versus star formation rate: theory confronts observations
Marta Volonteri, Pedro R. Capelo, Hagai Netzer +3
We use a suite of hydrodynamical simulations of galaxy mergers to compare star formation rate (SFR) and black hole accretion rate (BHAR) for galaxies before the interaction ('stoch…