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Comparison of optical appearance and infrared emission of extended dust clouds

  • C. P. de Vries
Part I: Nearby Molecular Clouds as Part of Larger Structure
Part of the Lecture Notes in Physics book series (LNP, volume 237)

Abstract

Several methods exist to observe interstellar dust. In this paper, some regions are selected of which optical appearance, like extinction and surface brightness, are discussed, together with a prelimenary comparison of infrared (100 μm ) emission. Careful comparison of extinction, reflection and IR-emission can yield information on the radiative properties of interstellar dust and of the interstellar radiation field.

Keywords

Surface Brightness Radiative Property Dust Cloud Infrared Emission Interstellar Dust 
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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References

  1. Mattila, K., 1979, Astron. & Astroph. 78, 253Google Scholar
  2. Murdin, P., Penston, M.V., 1977, M.N.R.A.S. 181, 657Google Scholar
  3. van Rhijn, P.J., 1929, Publ. Kapteyn Astron. Lab., No. 43Google Scholar
  4. de Vries, C.P., 1984, Astronomical Photography 1984, Edinburgh ed. E. Sim and K. Ishida p. 311Google Scholar

Copyright information

© Springer-Verlag 1985

Authors and Affiliations

  • C. P. de Vries
    • 1
  1. 1.Sterrewacht LeidenNetherlands

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