Figure 2 (IMAGE)

Kavli Institute for the Physics and Mathematics of the Universe

Figure 2

Caption

The fitting of the new model with the Perseus Cluster, experimenting with supernova yield from this project and from the literature. With an improved prescription in stellar astrophysics, the Si and S overproduction becomes within the limits observed for the Perseus Cluster. At the same time, the underproduction of Ar and Ca is relieved. However, the fitting highlights new challenges, including the under- (over-)production of Mn (Ni), which are closely related to the Type Ia supernova explosions.

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Leung et al.

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