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Early Evolution of the Universe and its Present Structure

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Cover of 'Early Evolution of the Universe and its Present Structure'

Table of Contents

  1. Altmetric Badge
    Book Overview
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    Chapter 1 Keynote: Structure of the Universe
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    Chapter 2 X-Ray Sources of Cosmological Relevance
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    Chapter 3 The e + -e - Annihilation Line and The Cosmic X-Ray Background
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    Chapter 4 QSO Surveys and Quasar Evolution
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    Chapter 5 Automated Quasar Detection
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    Chapter 6 The Asiago Catalogue of Quasi Stellar Objects
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    Chapter 7 The Quasar Redshift Limit
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    Chapter 8 Energy Distribution and Variability of BL LAC Objects. The Cases of PKS 2155–304 and 3C 66A
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    Chapter 9 Long-Term Variability of Quasi-Stellar Objects, and their Distribution in the Hubble Diagram
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    Chapter 10 Radio-Source Evolution and the Redshift Cut-Off
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    Chapter 11 A Model for the Cosmological Evolution of Radio Sources
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    Chapter 12 Quasar Galaxies: Two-Dimensional Image Deconvolutions
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    Chapter 13 QSO Luminosities at λ 1 MM
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    Chapter 14 QSO Redshift Limit and Periodicity in a Fib Universe
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    Chapter 15 Unbiased Searches for Quasars Beyond a Redshift of 3.5
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    Chapter 16 The Problem of the Redshifts
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    Chapter 17 The Evolution of the Radio Galaxy Population as Determined from Deep Radio-Optical Surveys
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    Chapter 18 A 6-CM Deep Sky Survey
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    Chapter 19 Near Infrared Photometry of Faint Radio Galaxies
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    Chapter 20 Near Infrared and Radio Observations of Distant Galaxies
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    Chapter 21 Studies of Faint Field Galaxies
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    Chapter 22 JF Photometry of Fourteen Distant Rich Clusters of Galaxies
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    Chapter 23 Color Distribution of Faint Galaxies and Quasi-Stellar Objects
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    Chapter 24 Spectroscopy of Distant Galaxies in Clusters
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    Chapter 25 A Redshift Survey of Very Faint (B ≤ 22.5) Field Galaxies, Radio Sources, and Quasars
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    Chapter 26 Spectral Energy Distributions of Galaxies in Moderate Redshift Clusters
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    Chapter 27 Distortion of the Microwave Background by Dust from Population III
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    Chapter 28 Was the Big Bang Hot?
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    Chapter 29 On Population III Star Formation
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    Chapter 30 Search for Small Scale Anisotropy of the 3K Emission of the Universe
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    Chapter 31 New Limits to the Small Scale Fluctuations in the Cosmic Background Radiation
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    Chapter 32 10 to 60 Arcmin Fluctuations in the Cosmic Microwave Background
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    Chapter 33 Deep Radio Source Counts and Small Scale Fluctuations of the Microwave Background Radiation
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    Chapter 34 Measurement of the 3 K Cosmic Background Noise in the Far Infrared
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    Chapter 35 On the Large-Scale Anisotropy of the Cosmic Background Radiation in the Far Infrared
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    Chapter 36 Large-Scale Anisotropy at Centimeter Wavelengths
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    Chapter 37 Large-Scale Anisotropy of the Cosmic Relic Radiation in Spatially Open Cosmological Models
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    Chapter 38 Comments and Summary on the Cosmic Background Radiation
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    Chapter 39 Redshifts and Large Scale Structures
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    Chapter 40 The Center for Astrophysics Redshift Survey
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    Chapter 41 The Anglo-Australian Redshift Survey
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    Chapter 42 Catalogue of Radial Velocities of Galaxies
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    Chapter 43 The Southern Cluster Survey
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    Chapter 44 Catalogue of Clusters that are Members of Superclusters
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    Chapter 45 Characteristic Size of Superclusters
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    Chapter 46 Quasars and Superclusters
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    Chapter 47 Further Investigations on Possible Correlations between QSOs and the Lick Catalogue of Galaxies
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    Chapter 48 Survey of the Bootes Void
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    Chapter 49 On the Origin of the Voids
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    Chapter 50 Properties of Galaxies in Low Density Regions
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    Chapter 51 Dynamics of Voids and Clusters and Fluctuations in the Cosmic Background Radiation
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    Chapter 52 Condensations and Cavities
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    Chapter 53 Correlation Functions, Microwave Background, and Pancakes
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    Chapter 54 A Photometric and Morphological Investigation of Very Remote Clusters
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    Chapter 55 Supernovae as a Cosmological Tool
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    Chapter 56 Substructure in Clusters of Galaxies
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    Chapter 57 Filaments
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    Chapter 58 Morphology of the Local Supercluster
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    Chapter 59 The Kinematics of the Local Supercluster
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    Chapter 60 Superclusters as Nondissipative Pancakes
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    Chapter 61 The Motion of the Local Group of Galaxies with Respect to the Background of Galaxies
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    Chapter 62 Infall of Galaxies into the Virgo Cluster
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    Chapter 63 Diameters of HI Disks in Virgo Cluster — And Field Galaxies
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    Chapter 64 Evidence of Intrinsic Correlation between the Luminosity and the Velocity Dispersion in Galaxy Groups
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    Chapter 65 Structure of Neighboring Superclusters: A Quantitative Analysis
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    Chapter 66 The Perseus Supercluster
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    Chapter 67 The Ursa Major Supercluster
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    Chapter 68 Dynamics of Some Remote Superclusters
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    Chapter 69 A2197 + A2199 Supercluster Region
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    Chapter 70 The Indus Supercluster
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    Chapter 71 The Southwest Extension of the Perseus Supercluster
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    Chapter 72 The Horologium Supercluster
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    Chapter 73 Unseen Mass
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    Chapter 74 Neutrino Mass and Galaxy Formation
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    Chapter 75 Massive Neutrinos and Ultraviolet Astronomy
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    Chapter 76 What does the Dynamical Analsis of Clusters of Galaxies Tell Us about Massive Neutrinos?
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    Chapter 77 Multimass Models for Clusters of Galaxies
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    Chapter 78 Perturbations in the Universe with Massive “...Inos”
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    Chapter 79 Black Holes and the Fate of a Closed Universe
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    Chapter 80 The [ An ]Isotropy of the X-Ray Sky
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    Chapter 81 Hot Accretion Disks and the High Energy Background
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    Chapter 82 X-Ray Observations of Active Galactic Nuclei
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    Chapter 83 QSO Absorption Lines
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    Chapter 84 Absorption Structure in the BL Lac Object 0215+015 at 20 km s -1 Resolution
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    Chapter 85 High-Redshift Molecular Clouds and Absorption-Line Spectra of Quasars
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    Chapter 86 The Statistic Study of Lα Absorption Lines
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    Chapter 87 Absorption-Line Spectroscopy of Close Pairs of QSOs
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    Chapter 88 Evolutionary Effect in Quasars as a Consequence of Galaxy Formation Process
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    Chapter 89 Are QSOs Gravitationally Lensed?
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    Chapter 90 Can All Quasars be Gravitationally Lensed Sy’s Nuclei ?
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    Chapter 91 Statistical Analysis of Optically Variable QSOs and Bright Galaxies: A Hint for Gravitational Lenses?
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    Chapter 92 Nature of ‘Unseen’ Galactic Envelopes
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    Chapter 93 The Theory of Large-Scale Structure of the Universe: Local Properties and Global Topology
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    Chapter 94 Self-Similar Gravitational Clustering
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    Chapter 95 Monte-Carlo Simulations of the Distribution of Faint Galaxies
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    Chapter 96 Neighboring Superclusters and their Environs
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    Chapter 97 Numerical Experiments on Galaxy Clustering
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    Chapter 98 Relativistic Stellar Dynamics
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    Chapter 99 Spherical and Toroidal Local Black Holes
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    Chapter 100 Possible Contraction of the Members of the Binary Pulsar PSR 1913+16 and its Astrophysical Consequences
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    Chapter 101 Observational Tests of Baryon Symmetric Cosmology
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    Chapter 102 Particle Phase Transitions can Prevent an Initial Cosmological Singularity
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    Chapter 103 Acceleration and Dissolution of Stars in the Antibang
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    Chapter 104 Inflationary Universe, Primordial Sound Waves and Galaxy Formation
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    Chapter 105 Phase Transitions of Cosmological Vacuum and Primordial Black Holes
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    Chapter 106 Unified Gauge Theories and Galaxy Formation
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    Chapter 107 Physics of the Bi-Partition of the Universe
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    Chapter 108 Causal Structure of the Early Universe
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    Chapter 109 R 2 Gravity and the Structure of the Universe
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    Chapter 110 The Strong Equivalence Principle and its Violation
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    Chapter 111 The Role of Particle Physics in Cosmology and Galactic Astronomy
Overall attention for this book and its chapters
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Title
Early Evolution of the Universe and its Present Structure
Published by
Springer Netherlands, December 2012
DOI 10.1007/978-94-009-7220-9
ISBNs
978-9-02-771662-0, 978-9-40-097220-9
Editors

Abell, G. O., Chincarini, G.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 2 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 2 100%

Demographic breakdown

Readers by professional status Count As %
Student > Bachelor 2 100%
Readers by discipline Count As %
Physics and Astronomy 2 100%