A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is
Measurements of the mass-to-light ratios of galaxies are crucial to a proper understanding of galaxy dynamics, dark matter distributions, and the general matter content of the universe. We report on results of a program to measure the change of theM/Lratio with redshift. Since the evolution of theM/Lcan be parameterized asdoi:10.1017/s0074180900233779 fatcat:o3g3xhjblnhxvjd2fmgp37ltku