Reprinted with kind permission from , 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
INTRODUCTION
- OVERVIEW
- Construction of Samples for Analysis
- The Limitations of Galaxy Catalogs
- Summary of Results
- DISCUSSION OF GALAXY PROPERTIES
- Optical Colors
- Optical Linear Size
- Optical Luminosity
- Optical Surface Brightness
- Far
Infrared Emission
- Radio Continuum Emission
- X-ray Emission
- Neutral Hydrogen Content
- Carbon Monoxide Content
- H
II Regions
- Chemical Abundances
- Total Masses and Related Quantities
- VARIATIONS IN GALAXY PROPRERTIES
- Global Properties
- The
Effect of Environment
- The
S0 Problem
-
Classical versus Dwarf
- SUMMARY
- REFERENCES
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.
