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, Kraft, Ralph P., Hernquist, Lars, Gilfanov, Marat, Churazov, Eugene, Genel, Shy, Forman, William R., Murray, Stephen S., Vikhlinin, Alexey, Jones, Christine, Böhringer, Hans, Bogdan, Akos, Torrey, Paul A.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/98311
https://orcid.org/0000-0001-8593-7692
https://orcid.org/0000-0002-5653-0786

Internet

http://hdl.handle.net/1721.1/98311
https://orcid.org/0000-0001-8593-7692
https://orcid.org/0000-0002-5653-0786

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