Proceedings of IAU Symposium No. 58 held in Canberra, Australia, August 12-15, 1973This is shown directly by a redshift-distance diagram recently prepared by Sandage and Tammann for Sc i galaxies. ... Plots of redshift versus angular size for brightest cluster galaxies (Sandage, 1972c) also have the correct slope for this ... A repetition of the test proposed by Hubble and Tolman (1935), which involves a correlation of surface brightness and redshift, would be important in this connection.
|Title||:||The Formation and Dynamics of Galaxies|
|Publisher||:||Springer Science & Business Media - 1974-09-30|