Introduction to Galaxy Formation and Evolution: From Primordial Gas to Present-Day Galaxies

Elliptical, spiral, and irregular galaxies are large systems made of stars, gas, and dark matter. This textbook explains the key physical processes of galaxy formation, from cosmological recombination to evolution, in a logical sequence. It introduces cosmology, illustrates the properties of galaxies, and explains the physical processes behind their formation. It also discusses how to find distant galaxies and extract their physical and evolutionary properties.

Format: Hardback
Length: 582 pages
Publication date: 17 October 2019
Publisher: Cambridge University Press

Galaxies, those captivating celestial entities, are vast systems composed of stars, gas, and dark matter. These remarkable structures have evolved over an astounding fourteen billion years since the Big Bang, shaped by a multitude of physical processes. This comprehensive textbook, designed to bridge the gap between introductory and specialized texts, delves into the intricate mechanics of galaxy formation. It unravels the key physical mechanisms that have shaped the galaxies we observe today, from the cosmic dance of primordial gas to the remarkable diversity of shapes and forms.

The book begins with an introduction to cosmology, providing a foundation for understanding the grand scale of the universe. It then showcases the captivating properties of galaxies in our present-day universe, painting a vivid picture of the vastness and complexity of the cosmos.

Next, the book delves into the intricate physical processes that govern galaxy formation. It explores the cosmic interplay of dark matter, gas, and gravity, shedding light on the intricate dance of matter and energy that shapes the universe. With a focus on the latest developments in this field, the text provides a comprehensive understanding of the complex mechanisms at play.

As the journey unfolds, the text concludes with practical insights on how to find distant galaxies and extract their physical and evolutionary properties through imaging and spectroscopic data. It offers a roadmap for astronomers and astrophysicists alike, guiding them in their quest to unravel the mysteries of the cosmos.

In essence, this textbook serves as a valuable resource for anyone seeking to delve deeper into the fascinating world of galaxies. It provides a comprehensive and up-to-date account of the key physical processes of galaxy formation, offering a deeper understanding of the cosmos and its incredible diversity of celestial wonders.

Weight: 1394g
Dimension: 196 x 253 x 32 (mm)
ISBN-13: 9781107134768