Understanding the Physical Processes Driving Galaxy Evolution in Clusters: A Case Study of Two z ~ 0.5 Galaxy Clusters

Understanding the Physical Processes Driving Galaxy Evolution in Clusters: A Case Study of Two z ~ 0.5 Galaxy Clusters

<p>Clusters of galaxies represent the largest laboratories in the universe for testing the incredibly chaotic physics governing the collapse of baryons into the stars, galaxies, groups, and diffuse clouds that we see today. Within the cluster environment, there are a wide variety of physical p...

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Bibliographic Details
Main Author: Moran, Sean Michael
Format: Others
Published: 2008
Online Access:https://thesis.library.caltech.edu/3182/1/thesis_final.pdf
Moran, Sean Michael (2008) Understanding the Physical Processes Driving Galaxy Evolution in Clusters: A Case Study of Two z ~ 0.5 Galaxy Clusters. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/C7Q1-DF25. https://resolver.caltech.edu/CaltechETD:etd-08212007-151300 <https://resolver.caltech.edu/CaltechETD:etd-08212007-151300>

Internet

https://thesis.library.caltech.edu/3182/1/thesis_final.pdf
Moran, Sean Michael (2008) Understanding the Physical Processes Driving Galaxy Evolution in Clusters: A Case Study of Two z ~ 0.5 Galaxy Clusters. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/C7Q1-DF25. https://resolver.caltech.edu/CaltechETD:etd-08212007-151300 <https://resolver.caltech.edu/CaltechETD:etd-08212007-151300>

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