Titlebook: Extragalactic Astronomy and Cosmology; An Introduction Peter Schneider Textbook 20061st edition Springer-Verlag Berlin Heidelberg 2006 Cosm

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書(shū)目名稱Extragalactic Astronomy and Cosmology影響因子(影響力)




書(shū)目名稱Extragalactic Astronomy and Cosmology影響因子(影響力)學(xué)科排名




書(shū)目名稱Extragalactic Astronomy and Cosmology網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Extragalactic Astronomy and Cosmology網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Extragalactic Astronomy and Cosmology被引頻次




書(shū)目名稱Extragalactic Astronomy and Cosmology被引頻次學(xué)科排名




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書(shū)目名稱Extragalactic Astronomy and Cosmology讀者反饋




書(shū)目名稱Extragalactic Astronomy and Cosmology讀者反饋學(xué)科排名

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Informationsintegration in Biodatenbankenearly 8000 objects, most of them galaxies. In 1912, Vesto Slipher found that the spiral nebulae are rotating, using spectroscopic analysis. But the nature of these extended sources, then called nebulae, was still unknown at that time; it was unclear whether they are part of our Milky Way or outside it.

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garrulous

The World of Galaxies,early 8000 objects, most of them galaxies. In 1912, Vesto Slipher found that the spiral nebulae are rotating, using spectroscopic analysis. But the nature of these extended sources, then called nebulae, was still unknown at that time; it was unclear whether they are part of our Milky Way or outside it.

古老

tic astronomy and proven textbook author.Fills a need for a .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. Then, from

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fulmination

Cosmology I: Homogeneous Isotropic World Models,e Universe is homogeneous when averaged over large spatial scales. Aspects of inhomogeneous cosmology, and thus the formation and evolution of structures in the Universe, will be considered later in Chap. 7.