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Physical Processes in the Large Scale ISM from Dust Observations

Published online by Cambridge University Press:  25 May 2016

F. Boulanger
F. Boulanger*
Affiliation:
Institut d'Astrophysique Spatiale, Université Paris, France

Abstract

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Over the last two decades observations of dust emission in the infrared have played an important role in the development of research on the interstellar medium. The study of the spectral energy distribution has led to the discovery of small dust particles including the large aromatic molecules (PAHs). Infrared sky images have been used to study the structure of interstellar matter, the evolution of dust within the interstellar medium and the star formation efficiency of interstellar clouds.

Type
Part 3. The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 153 - 164
Copyright
Copyright © Kluwer 1998 

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