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Properties of E & S0 Galaxies in the Coma Cluster
1996
Symposium - International astronomical union
As one of the richest nearby clusters, Coma is the ideal place to study the structure of galaxies as a function of environmental density, thus to constrain the theories of galaxy formation and evolution. For a magnitude limited sample of ≈ 40 E and S0 galaxies we want to obtain spectra with sufficient S/N and spatial resolution, that we can derive the rotation curves, the velocity dispersions profiles and the radial gradients of the line indices of Mg, Fe and Hβ. Following questions will be
doi:10.1017/s007418090023338x
fatcat:j42xvoavfnh5vod34lfhkgxitm