The magnitudes and surface brightnesses were also k-corrected. For Johnson B and U we used the k-correction given by Pence (1976), see Table . We used a linear interpolation in . All the HydraI galaxies have in the range 0.00-0.02. For Gunn r we used the k-correction from JFK92. The value at is listed in Table for comparison with Johnson B and U. For the 8 galaxies without a measured redshift, the cluster mean of = 3718 km/s (Zabludoff et al. 1990) was used. The k-corrections for the HydraI galaxies are given in Table .
Properties of E and S0 Galaxies in the Clusters HydraI and Coma
Master's Thesis, University of Copenhagen, July 1997
Bo Milvang-Jensen (email@example.com)