Morphological Astronomy

Man has a great tendency to get lost or to hide, as the case may be, in a jungle of details and in unnecessary complications. Why do anything simply if you can do it complicated? And still, life itself presents a sufficient number of problems to keep us busy. There would seem to be no need to create...

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Bibliographic Details
Main Author: Zwicky, Fritz
Format: eBook
Language:English
Published: Berlin, Heidelberg Springer Berlin Heidelberg 1957, 1957
Edition:1st ed. 1957
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
Table of Contents:
  • 17. Review of the Observations on the Clusters of Galaxies in Coma, Cancer and Pegasus
  • 18. Irregular Clusters of Galaxies
  • 19. Isopleths of Nebular Distribution
  • III: The Large Scale Distribution of Galaxies and of Clusters of Galaxies
  • 20. Past and Present Views
  • 21. Cluster Cells
  • 22. The Field of the Coma Cluster
  • 23. The Field of the Pegasus Cluster
  • 24. The Field of the Corona Borealis Cluster
  • 25. Various Statistical Methods in the Field of Dimensionless Morphology. Contagion
  • 26. Comparison of the Observed and of the Random Distribution Curves of Galaxies
  • 27. Intergalactic Obscuration
  • 28. Counts of Galaxies in Depth and in Width
  • 29. Counts of Galaxies in Dependence upon Apparent Magnitude
  • IV: Kinematic and Dynamic Characteristics of the Large Scale Aggregates of Matter
  • 30. The Velocities of Galaxies
  • 31. Some Basic Problems Relating to the Universal Redshift
  • 32. Elements of a Theory of the Large Scale Distribution of Matter in the Universe
  • 33. Dimensional Aspects of Large Scale Clustering
  • 34. Hydrodynamical Concepts
  • 35. Applications of the Virial Theorem to Clusters of Galaxies
  • 36. Clusters of Galaxies and the Emden Gravitational Isothermal Gas Sphere
  • 37. A Possible Universal Characteristic Central Density of Clusters of Galaxies
  • 38. Relative Physical Characteristics of Galaxies and of Clusters of Galaxies
  • V: Dimensional and Dimensionless Morphology in Cosmology
  • 39. Appraisal of Past Approaches to the Exploration of Extragalactic Space
  • 40. Methodology of Cosmological Research
  • 41. Distribution of Clusters of Galaxies and their Apparent Populations. Intergalactic Obscuration
  • 42. The Frequency of Clusters of Galaxies as a Function of their Angular Diameters. Crucial Tests for the Theory of the Expanding Universe
  • 43. The Total Space Occupied by the Large Clusters of Galaxies
  • I: Morphological Research and Invention
  • 1. Introductory Remarks
  • 2. Random Intuition and Systematized Discovery, Research and Invention. Communicable Truth and Incommunicable Truth
  • 3. The Formalism of Communicable Truth
  • 4. The Method of Negation and Subsequent Construction
  • 5. The Morphological Method of Analysis and Construction
  • 6. Past Applications of the Morphological Method
  • 7. Deficiencies which Aid the Morphological Method
  • 8. The Record of the 18-inch Schmidt Telescope on Palomar Mountain
  • 9. Specific Plans for a Morphological Approach to Astronomy
  • II: Clouds and Clusters of Galaxies
  • 10. The Known and the Unknown
  • 11. The Large Scale Distribution of Matter in the Universe
  • 12. The Coma Cluster of Galaxies
  • 13. Excursion into the Theory of Probabilities
  • 14. Continuation of the Discussion on the Coma Cluster
  • 15. The Cancer Cluster of Galaxies
  • 16. The Pegasus Cluster of Galaxies
  • 60. Astrophysical Theories
  • 61. Material Reconstruction of Parts of the Universe
  • 62. Sociological Problems
  • VIII: The Morphological Method and a priori Knowledge. The Magic Numbers
  • 63. Philosophy and Communicable Truth
  • 64. The Irreducible Foundations of Communicable Truth
  • 65. Some Specific Problems
  • 66. Outstanding Transcendental Numbers
  • 67. The Dimensionalities used in Physics
  • 68. Why is Space Three-Dimensional?
  • 69. Other Magic Numbers
  • 70. The Nature of the Physical Laws
  • Epilogue
  • Namelndex
  • 44. The Luminosity Function of Cluster Galaxies
  • 45. Preliminary Test of the Theory of a Flat Expanding Universe
  • 46. The Morphological Approach Toward the Determination of Absolute Dimensions and of Absolute Physical Characteristics of Very Remote Objects
  • 47. Remarks on the Morphology of Possible Cosmological Theories
  • 48. The Einstein Redshift
  • 49. The Gravitational Drag of Light
  • VI: Morphological Features of Individual Galaxies
  • 50. References to the History of the Subject
  • 51. Program for the Investigation of Individual Galaxies by the Methods of Dimensionless Morphology
  • 52. The Kinematic and Dynamic Characteristics of Galaxies
  • 53. The Masses of Galaxies
  • 54. Galaxies as Gravitational Lenses
  • 55. The Luminosity Function of Galaxies
  • 56. Multiple Galaxies and Intergalactic Matter
  • VII: Morphological Astronomical Kaleidoscope
  • 57. General Remarks
  • 58. Observations Made and Planned
  • 59. Experimentation with Celestial Objects