The Astrophysical Journal, Supplement Series
Department of Physics and Astronomy
The long-slit spectra obtained along the minor axis, offset major axis, and diagonal axis are presented for 12 E and S0 galaxies of the Coma Cluster drawn from a magnitude-limited sample studied before. The rotation curves, velocity dispersion profiles, and the H3 and H4 coefficients of the Hermite decomposition of the line-of-sight velocity distribution are derived. The radial profiles of the Hβ, Mg, and Fe line strength indices are measured too. In addition, the surface photometry of the central regions of a subsample of four galaxies recently obtained with the Hubble Space Telescope is presented. The data will be used to construct dynamical models of the galaxies and study their stellar populations.
Dartmouth Digital Commons Citation
Corsini, E. M.; Wegner, G.; Saglia, R. P.; and Thomas, J., "Spatially Resolved Spectroscopy of Coma Cluster Early‐Type Galaxies. IV. Completing the Data Set" (2008). Dartmouth Scholarship. 2303.