ARlogo Annu. Rev. Astron. Astrophys. 1994. 32: 115-52
Copyright © 1994 by Annual Reviews. All rights reserved

Reprinted with kind permission from Annual Reviews, 4139 El Camino Way, Palo Alto, California, USA


PHYSICAL PARAMETERS ALONG THE HUBBLE SEQUENCE

Morton S. Roberts

National Radio Astronomy Observatory 1, Charlottesville, VA 22903

Martha P. Haynes

Center for Radiophysics and Space Research and National Astronomy and Ionosphere Center 2, Cornell University, Ithaca, NY 14853 and National Radio Astronomy Observatory, Green Bank, WV 24944


Key words: galaxies, physical properties, morphological type, mass, star formation


Table of Contents



1 The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under a cooperative agreement with the National Science Foundation.
2 The National Astronomy and Ionosphere Center is operated by Cornell University under a cooperative agreement with the National Science Foundation.

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