Titlebook: Galaxy Formation; Malcolm S. Longair Textbook 2023Latest edition The Editor(s) (if applicable) and The Author(s), under exclusive license

Johnson

書目名稱Galaxy Formation影響因子(影響力)




書目名稱Galaxy Formation影響因子(影響力)學(xué)科排名




書目名稱Galaxy Formation網(wǎng)絡(luò)公開度




書目名稱Galaxy Formation網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Galaxy Formation被引頻次




書目名稱Galaxy Formation被引頻次學(xué)科排名




書目名稱Galaxy Formation年度引用




書目名稱Galaxy Formation年度引用學(xué)科排名




書目名稱Galaxy Formation讀者反饋




書目名稱Galaxy Formation讀者反饋學(xué)科排名

不安

The Large Scale Structure of the Universeion (CMB) over the sky and its spectrum. The remarkable isotropy of the CMB contrasts with large-scale distribution of galaxies which display huge walls and voids on large scales, which has a sponge-like topology. Their distributions are described by correlation functions. Combining Hubble’s law wit

Disk199

Galaxies, interacting, starburst and active galaxies. Correlations among the populations of galaxies include the red and blue sequences, colour versus absolute magnitude, the light distribution in galaxies and the Sérsic Index. Correlations among their spectroscopic and gaseous properties include mean stell

北極人

Filibuster

The Theoretical Frameworkrelating observables to the intrinsic properties of the objects studied. The application of the cosmological principle and the development of the metric for isotropic curved spaces leads to the Robertson-Walker metric. This metric provides the tool for understanding the significance of the cosmologi

藝術(shù)

An Introduction to Relativistic Gravityprovides insights into how it differs from Newtonian gravity. The theory is based upon the Principle of Equivalence which leads to the gravitational redshift and the bending of light rays in curved space-time. Detailed tests of the theory involve Parameterised Post-Newtonian (PPN) models for the fou

藝術(shù)

擔(dān)憂

The Determination of Cosmological Parametersot the predictions of the models are in accord with observations of the extragalactic Universe. First, we parameterise the predictions of the models with quantities we might hope to measure. The classical cosmological tests in which standard properties galaxies and other extragalactic objects are de

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Legend

Nucleosynthesis in the Early Universelving the problem of the present day abundances of the light elements. First, we need to establish the equilibrium abundances of all species which contribute to the inertial mass density of the Universe and how it changes with cosmic epoch. This involves understanding how weakly interacting particle