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Far-Infrared and Submillimeter Observations of Interstellar Clouds

Published online by Cambridge University Press:  04 August 2017

Gary Melnick
Gary Melnick*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA (USA) 02138

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This paper reviews a number of ways in which the results of far-infrared and submillimeter (FIR/SMM) observations (50 μm ≤ λ ≤ 1 mm) have been used to address some of the important questions in astrochemistry. On scales of kiloparsecs these might include questions of abundance gradients; on scales of parsecs these might include questions about the chemical structure of molecular clouds; and on scales of tenths of parsecs or less, these might include questions about chemical processing in shocks.

Type
Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 137 - 152
Copyright
Copyright © Reidel 1987 

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