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Ionization fronts as phase transitionsModel weak D-type ionization fronts have been constructed which include the effects of magnetic pressure and H I coolants. Ly-alpha cooling is found to suppress the high-temperature peak of 15,000 to 20,000 K found in earlier models. Ionization fronts are found to be closely related to phase transitions.
Document ID
19770045112
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/155091
Authors
Hill, J. K. (National Radio Astronomy Observatory Charlottesville, Va., United States)
Date Acquired
August 8, 2013
Publication Date
March 15, 1977
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
77A27964
Funding Number(s)
CONTRACT_GRANT: NSF AST-75-02181
CONTRACT_GRANT: NGR-05-003-578
Distribution Limits
Public
Copyright
Other

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