next previous
Up: Kinematical data on early-type IV.


1 Introduction

We have recently begun to present kinematical measurements from absorption spectroscopy on early-type galaxies (Simien & Prugniel 1997a,b, and c: hereafter Papers I, II, and III, respectively); these data are intended to contribute to the study of several structural and evolutionary issues. As part of our continuous effort to get reliable velocity dispersions and rotation curves on a statistically significant sample of objects, we presently report on observations on a fourth list of targets.

This work follows closely the technique already described in full detail in Paper I, for both observation and reduction, and only a minimum of explanations will be given here.


next previous
Up: Kinematical data on early-type IV.

Copyright The European Southern Observatory (ESO)