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Titlebook: Extragalactic Astronomy and Cosmology; An Introduction Peter Schneider Textbook 2015Latest edition Springer-Verlag GmbH Germany, part of Sp

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发表于 2025-3-21 17:02:22 | 显示全部楼层 |阅读模式
书目名称Extragalactic Astronomy and Cosmology
副标题An Introduction
编辑Peter Schneider
视频video
概述Widely expanded second edition of this leading astronomy textbook now incorporates some of the most spectacular results from new observatories like the Galaxy Evolution Explorer, Herschel, ALMA, WMAP
图书封面Titlebook: Extragalactic Astronomy and Cosmology; An Introduction Peter Schneider Textbook 2015Latest edition Springer-Verlag GmbH Germany, part of Sp
描述.This second edition has been updated and substantially expanded. Starting with the description of our home galaxy, the Milky Way, this cogently written textbook introduces the reader to the astronomy of galaxies, their structure, active galactic nuclei, evolution and large scale distribution in the Universe. After an extensive and thorough introduction to modern observational and theoretical cosmology, the focus turns to the formation of structures and astronomical objects in the early Universe. The basics of classical astronomy and stellar astrophysics needed for extragalactic astronomy are provided in the appendix..While this book has grown out of introductory university courses on astronomy and astrophysics and includes a set of problems and solutions, it will not only benefit undergraduate students and lecturers; thanks to the comprehensive coverage of the field, even graduate students and researchers specializing in related fields will appreciate it as a valuable reference work..
出版日期Textbook 2015Latest edition
关键词Active Galactic Nuclei; Big Bang; Cosmic Microwave Background; Cosmology Textbook; Early Universe; Extrag
版次2
doihttps://doi.org/10.1007/978-3-642-54083-7
isbn_softcover978-3-662-50060-6
isbn_ebook978-3-642-54083-7
copyrightSpringer-Verlag GmbH Germany, part of Springer Nature 2015
The information of publication is updating

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发表于 2025-3-21 20:22:24 | 显示全部楼层
The Milky Way as a galaxy,ich we are able to study astrophysical processes in detail. Therefore, our journey through extragalactic astronomy will begin in our home Galaxy, with which we first need to become familiar before we are ready to take off into the depths of the Universe. Knowing the properties of the Milky Way is in
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Cosmology I: Homogeneous isotropic world models,instead we will turn our attention to the space and time in which these objects are embedded. These considerations will then lead to a world model, the model of our cosmos. We need such a model also to interpret the observations of distant objects, i.e., those with a redshift for which the local Hub
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Cosmology II: Inhomogeneities in the Universe,ption of a (spatially) homogeneous and isotropic universe. Of course, the assumption of homogeneity is justified only on large scales because observations show us that our Universe is inhomogeneous on small scales—otherwise no galaxies or stars would exist.
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The Universe at high redshift, This might have given the impression that, with the determination of the values for .., .. etc., cosmology is nearing its conclusion. As a matter of fact, for several decades cosmologists have considered the determination of the density parameter and the expansion rate of the Universe as their prim
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Outlook, understanding of astrophysical processes, which in turn is driven by observational results. It is easy to foresee that the evolution of instrumental capabilities will continue rapidly in the near future, enabling us to perform better and more detailed studies of cosmic sources. Before we will menti
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