Galaxies are the fundamental units of cosmic matter that make up the universe and they change in remarkable ways over 13.7 billion years of cosmic time. We are just now discovering how galaxies we can see over these billions of years are evolving from small, star forming systems to larger, more massive and passive systems at later times. One of the ways that this process is seen in through the resolved structures of galaxies - that is, the shape and form of galaxies.
This book explains the structural evolution of galaxies, how we measure it, how these measurements change with time, and how observing this reveals important information about galaxy formation and evolution. This includes how the general forms of galaxies change with time as well as uncovering the methods for producing structural changes, especially those involving galaxy mergers. The book also explains the future of the field through the use of machine learning tools, and how galaxy structure can be used as a new approach to measure unique features of the universe, such as cosmological properties and parameters.
This book explains the structural evolution of galaxies, how we measure it, how these measurements change with time, and how observing this reveals important information about galaxy formation and evolution. This includes how the general forms of galaxies change with time as well as uncovering the methods for producing structural changes, especially those involving galaxy mergers. The book also explains the future of the field through the use of machine learning tools, and how galaxy structure can be used as a new approach to measure unique features of the universe, such as cosmological properties and parameters.
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