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- W3100471411 abstract "Evidence supporting the hypothesis of an invariant stellar initial mass function (IMF) is strong and varied. The intracluster medium (ICM) in rich clusters of galaxies is one of the few contrary locations where recent interpretations of the chemical abundances have favored an IMF that is biased toward massive stars, compared with the normal IMF. This interpretation hinges upon the neglect of Type Ia supernovae toward the ICM enrichment, and a particular choice of the nucleosynthesis yields of Type II supernovae. We demonstrate here that when one adopts yields determined empirically from observations of Galactic stars, rather than the uncertain model yields, a self-consistent picture may be obtained with an invariant stellar IMF and about half of the iron in the ICM being produced by Type Ia supernovae." @default.
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- W3100471411 date "1997-11-20" @default.
- W3100471411 modified "2023-09-26" @default.
- W3100471411 title "The Intracluster Medium: An Invariant Stellar Initial Mass Function" @default.
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- W3100471411 doi "https://doi.org/10.1086/311021" @default.
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