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| Naji, M. |
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| Motta, Antonella |
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| Aletan, Dirar |
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| Mohamed, Tarek |
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| Ertürk, Emre |
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| Taccardi, Nicola |
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| Petrov, R. H. | Madrid |
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| Casati, R. |
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| Kočí, Jan | Prague |
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| Kalteremidou, Kalliopi-Artemi | Brussels |
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| Azam, Siraj |
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| Ospanova, Alyiya |
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| Ali, M. A. |
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| Popa, V. |
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| Rančić, M. |
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| Ollier, Nadège |
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| Azevedo, Nuno Monteiro |
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| Landes, Michael |
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Bulbul, G. Esra
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document
Constraining SNe Enrichment Using X-ray Observations of Clusters of Galaxies
Abstract
X-ray spectroscopy yields accurate measurements of metal enrichment in the intra-cluster medium (ICM). The large reservoir of metals in clusters of galaxies provides a unique way to probe the total number and fraction of supernovae (SNe) types that enrich the ICM integrated over the cluster life-time by directly modeling high spectral resolution X-ray observations using various nucleosynthesis models. The XSPEC model, snapec, offering the possibility to use these vast reservoir of metals in clusters of galaxies to probe the supernovae rates and thereby test the SNe type Ia progenitor models. We will present the evolution of SNe type Ia rate obtained from the XMM-Newton observations of clusters of galaxies to constrain the possible SNe type Ia progenitors....