Evolution of Galaxies

Abstract

There have been several previous discussions of this subject (G. Burbidge [8],M. Burbidge [4], Sandage [34], Roberts [31]), and therefore we wish merelyto describe and review more recent ideas and work on the evolution of galaxies. It should be made clear at the outset that there is as yet no complete and satisfactory theory of the way in which a galaxy may evolve. However, the problem may be attacked in at least three distinct ways. (a) In what may be called the statistical method, one collects as much data as possible (of a kind involving observations that can be carried out on a large number of objects) about as many normal galaxies of all types as possible. Attempts can then be made to correlate the various measurements, in the hope that a consistent picture may emerge. (b) One may study those galaxies which present peculiarities suggesting that they may be in a stage that is likely to change in a time scale short compared with the Hubble time or the total lifetime of a galaxy. Various kinds of galaxies that are structurally peculiar fall into this category, also the radio galaxies. One may also measure in detail such things as velocity fields in particular galaxies where there seem to be motions other than simple circular rotation of an axially symmetric object under the action of gravitational forces alone. Work under this heading is necessarily carried out on relatively few objects; the aim is to deduce from the observations the way in which a particular galaxy may change from its present configuration to another one. (c) A purely theoretical approach may be made, with recourse to what isknown about related fields such as the theory of stellar evolution. Thus one could consider the way in which a proto-galaxy composed of hydrogen gas would gravitationally contract and form into stars, and what its subsequent historywould be after the first star formation began.

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Document Details

Document Type
Technical Report
Publication Date
Jan 01, 1967
Accession Number
AD1027227

Entities

People

  • E. M. Burbidge
  • G. R. Burbidge

Organizations

  • University of California, San Diego

Tags

Communities of Interest

  • Air Platforms
  • Biomedical

DTIC Thesaurus Topics

  • Angular Momentum
  • Electromagnetic Radiation
  • Equations
  • High Density
  • Line Spectra
  • Magnetic Fields
  • Materials
  • Military Research
  • Momentum
  • Observation
  • Observatories
  • Photographs
  • Photography
  • Stars
  • Steady State
  • Stellar Evolution
  • Stratified Fluids

Fields of Study

  • Physics

Readers

  • Astronomy/Astrophysics
  • Educational Psychology
  • Theoretical Analysis.