The Epoch of Galaxy Formation

Scientists in the late twentieth century are not the first to view galaxy formation as a phenomenon worthy of explanation in terms of the known laws of physics. Already in 1754 Kant regarded the problem as essentially solved. In his Univerlal Natural Hutory and Theory 0/ the H eaven$ he wrote; "...

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Bibliographic Details
Other Authors: Frenk, Carlos S. (Editor), Ellis, Richard S. (Editor), Shanks, T. (Editor), Heavens, Alan F. (Editor)
Format: eBook
Language:English
Published: Dordrecht Springer Netherlands 1989, 1989
Edition:1st ed. 1989
Series:Nato Science Series C:, Mathematical and Physical Sciences
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
Table of Contents:
  • I. Forming Galaxies
  • Galaxy formation: high redshift or low?
  • Observable signatures of young galaxies
  • A multicolor search for forming galaxies
  • Lyman-alpha galaxies in 1988
  • Morphological evolution of radio galaxies
  • High redshift radio galaxies and galaxy formation
  • Deep surveys of field and low-flux-radio galaxies
  • Constraints on the epoch of galaxy formation from deep U-band counts
  • II. Gas Clouds
  • Lyman line absorption systems
  • Damped Lyman alpha absorbers: the progenitors of galactic disks
  • A chemically young galaxy at z=2.3
  • Lyman ? emission from a possible primeval galaxy at z=2.5
  • III. Quasars
  • The quasar redshift cut-off
  • Fifty-three multicolour selected quasars with redshifts greater than three
  • The luminosity function and clustering of QSOs
  • High redshift quasars in the cold dark matter cosmology
  • The intergalactic medium and the epoch of galaxy formation
  • A cooling flow around the quasar 3C196
  • Simulations of the visual appearance of galaxy clusters at high redshift
  • Central galaxy formation by cooling flows
  • Constraints on the amplitude of primordial density fluctuations
  • Spottiness in the structure of the microwave background radiation
  • Energetic constraints on spectral distortions of the microwave background
  • CBR polarization by cosmic dust at high redshifts
  • Growth of perturbations in a collapsing protogalaxy
  • The turnaround epoch of clusters of galaxies
  • The correlations of peaks in random noise
  • Density maxima as sites for galaxy formation
  • A cross-correlation method to test the dependence of the clustering of galaxies on luminosity
  • Constraints on the formation redshift of bright galaxies inbiased scenarios
  • Biased theories with non-v threshold
  • Sinking satellites and disk heating of spiral galaxies
  • Galaxy formation in asymmetric dark haloes
  • Gas in a cosmological N-body simulation
  • Dissipational galaxy formation
  • Recent results on cosmic strings and galaxy formation
  • Galaxy formation in unstable dark matter models
  • VII. The Age of the Galaxy
  • The age of the Galaxy
  • The nature and age of the galactic thick disk
  • A simple model for the Local Group of Galaxies
  • VIII. Prospects
  • Future observational prospects
  • Poster Papers
  • A new deep AAT redshift survey
  • On the interpretation of galaxy counts, and color and redshift distributions
  • The interpretation of faint galaxy counts
  • Limits on dust in damped Lyman-alpha systems and the obscuration of quasars
  • The stellar content of early-type galaxies in dense environments
  • A new study of absorption line density in QSO’s Ly? forest
  • The Edinburgh/Durham southern galaxy catalogue
  • Mass-to-light ratios and the age of galaxies
  • Emission lines and star formation in radio galaxies
  • The age of the radiogalaxy 0902+34 at the redshift z=3.395
  • Statistics of radio galaxy populations and galaxy formation
  • IV. Evolution of Galaxies and Clusters
  • Galaxy evolution in high density environments
  • Evolution of compact groups and formation of elliptical
  • Properties of galaxy clusters associated with quasars
  • History of star formation in normal galaxies
  • Recurrent star formation in elliptical galaxies
  • V. Background Radiation
  • Constraints on galaxy formation from cosmic background radiations
  • Explaining the Nagoya-Berkeley submillimetre background
  • Star formation and the x-ray background
  • VI. Models
  • Galaxy formation and biased clustering
  • Galaxy clusters and the epoch of galaxy formation
  • Exploring origins for the Hubble sequence
  • Galaxy mergers in a CDM model
  • Clustering and dynamics in a dissipative CDM N-body simulation
  • The galaxy luminosity function: an alternative to the Press and Schechter technique
  • Galactic evolution and globalstar formation
  • Galaxy formation and cooling flows
  • The epoch of galaxy formation in explosion models
  • Tidal origin of starbursts and active galactic nuclei
  • The topology of large scale structure: observations
  • Append
  • Galaxy formation: the board game
  • Author Index