Probing the hot X-ray corona around the massive spiral galaxy, NGC 6753, using deep XMM-Newton observations
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...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
21 Nov 2017
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| In: |
Arxiv
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| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1710.07286
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| Verfasserangaben: | Akos Bogdan, Herve Bourdin, William R. Forman, Ralph P. Kraft, Mark Vogelsberger, Lars Hernquist, and Volker Springel |