Hydrodynamical simulations of early-type galaxies: effects of galaxy shape and stellar dynamics on hot coronae
Early-Type galaxies (ETGs) are embedded in hot (10^6-10^7 K), X-ray emitting gaseous haloes, produced mainly by stellar winds and heated by Type Ia supernovae explosions, by the thermalization of stellar motions and occasionally by the central super-massive black hole (SMBH). In particular, the ther...
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| Format: | Doctoral Thesis |
| Language: | en |
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Alma Mater Studiorum - Università di Bologna
2014
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| Online Access: | http://amsdottorato.unibo.it/6170/ |