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020 _a9781107134768
040 _cIIT Kanpur
041 _aeng
082 _a523.112
_bC49i
100 _aCimatti, Andrea
245 _aIntroduction to galaxy formation and evolution
_bfrom primordial gas to present-day galaxies
_cAndrea Cimatti, Filippo Fraternali and Carlo Nipoti
260 _bCambridge University Press
_c2020
_aCambridge
300 _aXiii, 571p
520 _aPresent-day elliptical, spiral and irregular galaxies are large systems made of stars, gas and dark matter. Their properties result from a variety of physical processes that have occurred during the nearly fourteen billion years since the Big Bang. This comprehensive textbook, which bridges the gap between introductory and specialized texts, explains the key physical processes of galaxy formation, from the cosmological recombination of primordial gas to the evolution of the different galaxies that we observe in the Universe today. In a logical sequence, the book introduces cosmology, illustrates the properties of galaxies in the present-day Universe, then explains the physical processes behind galaxy formation in the cosmological context, taking into account the most recent developments in this field. The text ends on how to find distant galaxies with multi-wavelength observations, and how to extract the physical and evolutionary properties based on imaging and spectroscopic data.
650 _aGalaxies -- Evolution
650 _aGalaxies -- Formation
700 _aFraternali, Filippo
700 _aNipoti, Carlo
942 _cBK
999 _c561182
_d561182