The Cosmic Evolution of Galaxy Structure
The Cosmic Evolution of Galaxy Structure by Christopher J. Conselice, published by IOP Publishing in 2020, offers an in-depth exploration of galaxies as fundamental units of cosmic matter. This edition, comprising 160 pages, delves into the remarkable changes galaxies undergo over 13.7 billion years, detailing their evolution from small, star-forming systems to larger, more massive structures. The book provides insights into how these structural changes are measured and the implications of these measurements for understanding galaxy formation and evolution.
Readers will find a comprehensive examination of the resolved structures of galaxies, including their shapes and forms, and how these evolve over time. The text discusses the processes behind structural changes, particularly those resulting from galaxy mergers, and highlights the role of machine learning tools in advancing the field. Additionally, it presents galaxy structure as a novel approach to uncovering unique features of the Universe, such as cosmological properties and parameters, making it a valuable resource for those interested in science, space science, and astronomy.
Official synopsis Publisher
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 the 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.
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