We present morphological type estimates, together with a detailed coded description for 59 galaxies in Coma and 80 in Perseus. The material for the morphological type estimates is adapted to the difficulty of morphological classification, ranging from Schmidt plates for obvious Ss to CCD data with a median restframe resolution of 0.65-0.75 Kpc for early-types.
In the present paper and in two previous ones (Paper I; Poulain
et al. 1992) we classify two magnitude complete samples of galaxies: all
(187) galaxies in Coma brighter than 
mag within 1 degree from the
cluster center and all (139) galaxies in Perseus brighter than 
mag in a box of 
. At the distance of these
two clusters, we sample an area of 17 and 91 Mpc2 and distances of up to
2.3 and 6.4 Mpc from the cluster center, for Coma and Perseus respectively,
and 4 to 5 orders of magnitude in galaxy density. The ranges of explored
clustercentric distances and galaxy densities allow us to study how the
cluster affects the galaxy properties. The results for Coma, based on these
data, are presented in Andreon (1996). For Perseus, work is in progress.
Acknowledgements
We thank Christian Pollas (Observatoire de Calern) for taking three Schmidt plates for this project, and Jean Guibert and his staff (MAMA) for digitizing the plates. We thank Bénédicte Rougeaux for her visual inspection of the OCA #2849 plate. This research made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration and of the Lyon-Meudon Extragalactic Database (LEDA) supplied by the LEDA team at the CRAL-Observatoire de Lyon (France). Skyeye (http://terra.ira.bo.cnr.it/ira/skyeye) greatly helped giving a quick and easy access to the Digitized Palomar Sky Survey