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The Detection of High Velocity Gas in Nearby Galaxies
Table of Contents
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The Detection of High Velocity Ga
What is HVG and why is it importa
What is HVG and why is it importa
Goals of the Project
140 Ft Observations
Selection Criteria
Observed Galaxies
Model Fitting
Details of Model Fitting
Details of Model Fitting
Details of Model Fitting
Details of Model Fitting
Results: Galaxies with Interferom
Results: Galaxies without Interfe
Summary
Summary
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Last update: 3/19/97