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The luminosity functions of taurus and chamaeleon

  • J. D. Hughes
  • J. P. Emerson
The Galaxy
Part of the Lecture Notes in Physics book series (LNP, volume 297)

Abstract

The Infrared Astronomical Satellite (IRAS) surveyed the sky at 12, 25, 60, and 100 µm providing an invaluable, unbiassed far-infrared database for the study of regions of active star formation. We obtain the far-infrared luminosity functions of Taurus and Chamaeleon, within which the stellar populations appear to be at a similar evolutionary stage (within statistical errors). We then convert the far-infrared luminosity functions to equivalent bolometric luminosity functions, and find a shortfall in the number of intermediate and high mass objects when we compared to the initial luminosity function for field stars (Miller and Scalo 1979).

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Copyright information

© Springer-Verlag 1988

Authors and Affiliations

  • J. D. Hughes
    • 1
  • J. P. Emerson
    • 1
  1. 1.Department of PhysicsQueen Mary CollegeLondon

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