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Preionization-dependent families of radiative shock wavesRadiation shock waves are shown to be organizable into families within which the spectra are very similar. A high-velocity shock into neutral material is spectrally similar to a somewhat slower shock in fully ionized material. The similarities should allow the identification of the family to which an observed spectrum belongs, while spectral details permit subsequent identification of the separate values of shock velocity and preionization. By calculating shock spectra for the various families at constant recombination zone density, rather than constant preshock density, it is possible to separate the effects of 'velocity' (by which is meant postionization enthalpy per atom) from those of 'density' (by which is meant the degree of collisional deexcitation in the optical lines).
Document ID
19860032508
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cox, D. P.
(Rice University Houston, TX, United States)
Raymond, J. C.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
November 15, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 298
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
86A17246
Funding Number(s)
CONTRACT_GRANT: NSF AST-84-15142
CONTRACT_GRANT: NGL-50-002-044
CONTRACT_GRANT: NAG5-87
Distribution Limits
Public
Copyright
Other

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