SIMBAD references

2012ApJ...748...48R - Astrophys. J., 748, 48 (2012/March-3)

Enhanced abundances in spiral galaxies of the Pegasus I cluster.

ROBERTSON P., SHIELDS G.A. and BLANC G.A.

Abstract (from CDS):

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.

Abstract Copyright:

Journal keyword(s): galaxies: abundances - galaxies: clusters: individual: Pegasus I - galaxies: evolution - galaxies: spiral - H II regions

Simbad objects: 31

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2020.02.19-07:53:21

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