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The mass function

  • I. Neill Reid
  • Suzanne L. Hawley
Part of the Astronomy and Planetary Sciences book series (PRAXIS)

Abstract

The number of stars per unit mass — the stellar mass function — describes how a molecular cloud redistributes its material to form stars. This parameter is also a necessary ingredient for determining the mass distribution and the total stellar mass in star clusters and external galaxies. It is therefore fundamental to both star-formation theory and Galactic structure.

Keywords

Star Formation Mass Function Cluster Member Stellar Mass Luminosity Function 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2000

Authors and Affiliations

  • I. Neill Reid
    • 1
  • Suzanne L. Hawley
    • 2
  1. 1.Formerly of Edinburgh UniversityEdinburghScotland
  2. 2.Department of Physics and AstronomyMichigan State UniversityEast LansingUSA

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