Roles of SNIa and SNII in ICM Enrichment
arXiv:astro-ph/9702036 · doi:10.1093/pasj/49.1.1
Abstract
Based on ASCA observations Mushotzky et al. (1996, ApJ 466, 686) have recently derived the relative-abundance ratios of -elements to iron, [α/Fe] \simeq 0.2-0.3N_{Fe}/N_H = 4.68 10^{-5}3.24 10^{-5}Δ[α/Fe] \simeq -0.16$ dex. By comparing the corrected [α/Fe] values with theoretical nucleosynthesis prescriptions of SNIa and SNII, we reach a conclusion that an SNIa iron contribution of 50% or higher in the ICM enrichment could not be ruled out, and might indeed be favoured based on the ASCA spectra.
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