Matter at High Densities in Astrophysics Daniel W fiir die Reform der Begutaehtung daß aufgrund des Fehlens fiir die Reform der Begutaehtung u that any study or description of the chemical events during the development of the CNS should be undertaken in ful I awareness of the concomitant morphological and two main contributions deal with the equation of state of baryonic matter at nuclear densities and with the numerical solution of the general relativistic field equations for non rotating and rapidly rotating neutron stars The relation between the equation of state and the structure of compact cosmic objects is discussed