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OH Masers

  • Moshe Elitzur
Part of the Astrophysics and Space Science Library book series (ASSL, volume 170)

Abstract

OH, the hydroxyl radical, holds the distinction of being both the first molecule detected in interstellar space at radio frequencies (Weinreb et al. 1963) and the first astronomical maser ever discovered (Weaver et al. 1965). This molecule still provides the largest variety of astronomical sources displaying maser activity. Strong OH maser emission is observed in both star-forming regions and late-type stars. Weak maser effects are prevalent in large molecular clouds and in comets as they circle around the sun. OH maser emission has also been detected in external galaxies. It is appropriate that OH masers be the first ones discussed in detail.

Keywords

Optical Depth Main Line Column Density Maser Emission Satellite Line 
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 Science+Business Media Dordrecht 1992

Authors and Affiliations

  • Moshe Elitzur
    • 1
  1. 1.Department of Physics and AstronomyUniversity of KentuckyLexingtonUSA

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