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Probing the hot X-ray corona around the massive spiral galaxy, NGC 6753, using deep XMM-Newton observations

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X-ray emitting gaseous coronae around massive galaxies are a basic prediction of galaxy formation models. Although the coronae around spiral galaxies offer a fundamental test of these models, observational constraints on their characteristics are still scarce. While the presence of extended hot coro...

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Bibliographic Details
Main Authors: Bogdán, Ákos (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2017 November 21
In: The astrophysical journal
Year: 2017, Volume: 850, Issue: 1
ISSN:1538-4357
DOI:10.3847/1538-4357/aa9523
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/1538-4357/aa9523
Verlag, kostenfrei, Volltext: http://stacks.iop.org/0004-637X/850/i=1/a=98
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Author Notes:Ákos Bogdán, Hervé Bourdin, William R. Forman, Ralph P. Kraft, Mark Vogelsberger, Lars Hernquist, and Volker Springel
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Probing the hot X-ray corona around the massive spiral galaxy, NGC 6753, using deep XMM-Newton observations by Bogdán, Ákos (Author) , Springel, Volker (Author) ,


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