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- W2067463708 abstract "We study the influence of cluster environment on the chemical evolution of spiral galaxies in the Pegasus I cluster. We determine the gas-phase heavy element abundances of six galaxies in Pegasus derived from H ii region spectra obtained from integral-field spectroscopy. These abundances are analyzed in the context of Virgo, whose spirals are known to show increasing interstellar metallicity as a function of H i deficiency. The galaxies in the Pegasus cluster, despite its lower density and velocity dispersion, also display gas loss due to interstellar-medium–intracluster-medium interaction, albeit to a lesser degree. Based on the abundances of three H i deficient spirals and two H i normal spirals, we observe a heavy element abundance offset of +0.13 ± 0.07 dex for the H i deficient galaxies. This abundance differential is consistent with the differential observed in Virgo for galaxies with a similar H i deficiency, and we observe a correlation between log (O/H) and the H i deficiency parameter DEF for the two clusters analyzed together. Our results suggest that similar environmental mechanisms are driving the heavy element enhancement in both clusters." @default.
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- W2067463708 date "2012-03-05" @default.
- W2067463708 modified "2023-09-26" @default.
- W2067463708 title "ENHANCED ABUNDANCES IN SPIRAL GALAXIES OF THE PEGASUS I CLUSTER" @default.
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- W2067463708 doi "https://doi.org/10.1088/0004-637x/748/1/48" @default.
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