HOT GASEOUS CORONAE AROUND SPIRAL GALAXIES: PROBING THE ILLUSTRIS SIMULATION

HOT GASEOUS CORONAE AROUND SPIRAL GALAXIES: PROBING THE ILLUSTRIS SIMULATION

The presence of hot gaseous coronae around present-day massive spiral galaxies is a fundamental prediction of galaxy formation models. However, our observational knowledge remains scarce, since to date only four gaseous coronae have been detected around spirals with massive stellar bodies ([> ove...

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Bibliographic Details
Main Authors: Vogelsberger, Mark (Contributor), Kraft, Ralph P. (Author), Hernquist, Lars (Author), Gilfanov, Marat (Author), Churazov, Eugene (Author), Genel, Shy (Author), Forman, William R. (Author), Murray, Stephen S. (Author), Vikhlinin, Alexey (Author), Jones, Christine (Author), Böhringer, Hans (Author), Bogdan, Akos (Author), Torrey, Paul A. (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), Torrey, Paul (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-09-01T20:28:53Z.
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