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

Johnson

书目名称Galaxy Formation影响因子(影响力)




书目名称Galaxy Formation影响因子(影响力)学科排名




书目名称Galaxy Formation网络公开度




书目名称Galaxy Formation网络公开度学科排名




书目名称Galaxy Formation被引频次




书目名称Galaxy Formation被引频次学科排名




书目名称Galaxy Formation年度引用




书目名称Galaxy Formation年度引用学科排名




书目名称Galaxy Formation读者反馈




书目名称Galaxy Formation读者反馈学科排名

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

北极人

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

艺术

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

艺术

担忧

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