图书简介
All matter, including galaxy clusters, galaxies, and their constituents follow orbits and flows driven by the net attraction of near and distant masses. The book presents the development of studies of peculiar motions along with discoveries in large-scale structure, the cosmic microwave background, baryonic oscillations, gravity waves, and their relation to current work on gravitation and dark matter.
The results of peculiar motion measurements in the late 20th century are described as they were used to search for the dipole of the galaxy motions, a determination of cosmic density, and to compare with the cosmic microwave dipole, which led to the discovery of galactic flows and the Great Attractor. Newer detailed measurements from surveys in the 21st century have helped resolve the nature of these structures. Some prospects for future investigations are discussed.
Key Features:
It gives a more detailed coverage of peculiar motions than other books including the distance scale, observational and bias corrections
It has a historical development of the discovery of peculiar motions up to their present state, not usually presented, and discusses other motions driven by gravity
It connects peculiar motions with other recent discoveries, including the cosmic microwave background, baryonic oscillations, gravity waves, etc. It could make a companion to more detailed technical treatises on these subjects
Foreword; List of Figures; Brief Historical Summary; Beginnings of Modern Astrophysics; Cosmological N-Body Simulations; Galaxy Evolution and Semi-Analytic Models; Early Developments on Large-Scale Structure; Unanswered Questions About Gravity; Magnitude Scale, Photometry, and Reddening; Types of Distances and Necessary Corrections to Data; Malmquist and Other Biases; Extragalactic Distance Ladder; Generation of Peculiar Velocities; Measurements and Analysis Methods of Distant Pecular Velocities; The Great Attractor and Peculiar Velocity Studies; Revolutions by CMB Studies; Baryonic Acoustic Oscillations; Gravitational Lensing; Motions of Binary Galaxy Clusters; Gravitational Radiation; 21st Century Peculiar Motion Studies; Conclusion;
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