We present the results of two-dimensional, grid-type hydrodynamical simulations, with parsec-scale central resolution, for the evolution of the hot gas in isolated early-type galaxies (ETGs).
AGN feedback and the origin and fate of the hot gas in early-type galaxies
Pellegrini, SilviaSupervision
;Ciotti, LucaSupervision
;
2020
Abstract
We present the results of two-dimensional, grid-type hydrodynamical simulations, with parsec-scale central resolution, for the evolution of the hot gas in isolated early-type galaxies (ETGs).File in questo prodotto:
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