Ghost Images in a Universe with Inhomogeneous Mass Distribution

Abstract

Abstract. An attempt is made to explain Morgan cD supergiant galaxies, the microwave background radiation and extended discrete radio sources as ghost images in a universe of strong positive curvature and inhomogeneous mass distribution.The observations of Humason et al. (1956), and of Minkowski (1960) and Baum (1962) revealed that up to z = 0.46 the Hubble plot of galaxies follows the equation B = 51ogz + 23.23 ±0.13.(1)The first