Are Gradients in Intracluster Metals and Galaxy Morphology Related?

Details Are Gradients in Intracluster Metals and Galaxy Morphology Related? Are Gradients in Intracluster Metals and Galaxy Morphology Related?

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...18510716d&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #107.16; Bulletin of the American Astronomical Society, Vol. 26, p.1499

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We present the preliminary results of a comparison between the morphological distribution of galaxies in clusters and the presence (or absence) of intracluster metal abundance gradients. The objective of such a comparison is to discriminate between possible metal injection mechanisms (e.g. winds, ram-pressure stripping) and sources (e.g. spirals, ellipticals and/or lenticulars).

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