Nearly Normal Galaxies

From the Planck Time to the Present

  • S. M. Faber
Conference proceedings

Part of the Santa Cruz Summer Workshops in Astronomy and Astrophysics book series (SANTA CRUZ)

Table of contents

  1. Front Matter
    Pages i-xxvi
  2. Stellar Evolution in Galaxies

    1. Front Matter
      Pages 1-1
    2. Jay A. Frogel
      Pages 3-9
    3. François Schweizer
      Pages 18-25
    4. Richard B. Larson
      Pages 26-35
    5. Carol J. Persson
      Pages 36-40
  3. Small Objects

    1. Front Matter
      Pages 45-45
    2. Marc Aaronson
      Pages 57-66
    3. Scott Tremaine
      Pages 76-77
  4. Galactic Structure and Dynamics: Observations

About these proceedings

Introduction

It is sometimes said that astronomy is the crossroads of physics. In the same spirit, it can forcefully be argued that galaxies are the crossroads of astronomy. Internal pro ces ses within galaxies involve all of the fundamental components of astrophysics: stellar evolution, star formation, low-density astrophysics, dynamics, hydrodynamics, and high-energy astrophysics. Indeed, one can hardly name an observational datum in any wavelength range on any kind of celestial object that does not provide a useful clue to galaxy formation and evolution. Although internal processes in galaxies until recently occupied most of our attention, we now know that it is also vital to relate galaxies to their environment. How galaxies congregate in larger structures and are in turn influenced by them are crucial questions for galactic evolution. On a grander level we have also come to regard galaxies as the basic building blocks of the universe, the basic units whereby the large­ scale structure of the universe is apprehended and quantified. On a grander level still, we also believe strongly that galaxies are the direct descendents of early density irregularities in the Big Bang. Galaxy properties are now viewed as providing a crucial constraint on the physics of the Big Bang and a vital link between the macroscopic and microscopic structure of the universe.

Keywords

Accretion Inflation Population Redshift Variation astronomy astrophysics early universe galaxies milky way observatory star star formation stellar evolution universe

Editors and affiliations

  • S. M. Faber
    • 1
  1. 1.Department of AstronomyUniversity of CaliforniaSanta CruzUSA

Bibliographic information

  • DOI https://doi.org/10.1007/978-1-4612-4762-3
  • Copyright Information Springer-Verlag New York 1987
  • Publisher Name Springer, New York, NY
  • eBook Packages Springer Book Archive
  • Print ISBN 978-1-4612-9145-9
  • Online ISBN 978-1-4612-4762-3
  • About this book