ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract We present the results of calculations of the hydrogen ionization fraction, non-LTE populations and corresponding line intensities in a large range of temperatures, densities, and external radiation fields, with emphasis on the conditions occurring in circumstellar shells. These calculations provide an extensive coverage of physical conditions for which no appropriate results are available in the current literature, and can be used as a guide for the detailed understanding of the formation of the hydrogen spectrum in cool, partially-ionized plasmas.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00646859
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