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, Silvia; Ciotti, Luca; Negri, Andrea; Ostriker, Jeremiah P.. - STAMPA. - 14:(2020), pp. 97-100. (Intervento presentato al convegno IAU Symposium S342: "Perseus in Sicily: From Black Hole to Cluster Outskirts" tenutosi a Noto, Italy nel May 2018) [10.1017/S1743921318003745].
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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