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Radical Formation, Chemical Processing, and Explosion of Interstellar Grains

  • J. Mayo Greenberg
Part of the Astrophysics and Space Science Library book series (ASSL, volume 55)

Abstract

The ultraviolet radiation in interstellar space is shown to create a sufficient steady state density of free radicals in the grain mantle material consisting of oxygen, carbon, nitrogen, and hydrogen to satisfy the critical condition for initiation of chain reactions. The criterion for minimum critical particle size for maintaining the chain reaction is of the order of the larger grain sizes in a distribution satisfying the average extinction and polarization measures. The triggering of the explosion of interstellar grains leading to the ejection of complex interstellar molecules is shown to be most probable where the grains are largest and where radiation is suddenly introduced; i.e. in regions of new star formation. Similar conditions prevail at the boundaries between very dark clouds and H II regions. When the energy released by the chemical activity of the free radicals is inadequate to explode the grain, the resulting mantle material must consist of extremely large organic molecules which are much more resistant to the hostile environment of H II regions than the classical dirty ice mantles made up of water, methane, and ammonia.

Keywords

Free Radical Star Formation Trap Site Interstellar Dust Interstellar Space 
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

© D. Reidel Publishing Company, Dordrecht, Holland 1976

Authors and Affiliations

  • J. Mayo Greenberg
    • 1
  1. 1.State University of New York and Dudley ObservatoryAlbany, New YorkUSA

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