The book begins by establishing the cosmological background and the role of dark matter, then moves to the formation of the first stars and galaxies. It examines how galaxies evolve through mergers, gas accretion, and the influence of supermassive black holes. The diversity of galaxy types, from spirals to ellipticals, is analyzed in relation to physical processes. The book concludes by exploring the large-scale distribution of galaxies within the cosmic web and the implications for the universe's future, drawing upon observational data and simulations.
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