Abstract
XMM-Newton recently discovered O VII line emission from ~ 2 million K gas near the outer parts of several clusters of galaxies. This emission is attributed to the Warm-Hot Intergalactic Medium. The original sample of clusters studied for this purpose has been extended and two more clusters with a soft X-ray excess have been found. We discuss the physical properties of the warm gas, in particular the density, spatial extent, abundances and temperature.
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Kaastra, J.S., Lieu, R., Tamura, T., Paerels, F.B.S., den Herder, J.W.A. (2004). XMM-Newton Discovery of O VII Emission from Warm Gas in Clusters of Galaxies. In: Lieu, R., Mittaz, J. (eds) Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena. Astrophysics and Space Science Library, vol 309. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2564-8_5
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DOI: https://doi.org/10.1007/978-1-4020-2564-8_5
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