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The structure of a shock wave traveling through a stellar atmosphere

✍ Scribed by I. A. Klimishin


Publisher
Springer
Year
1968
Tongue
English
Weight
651 KB
Volume
4
Category
Article
ISSN
0571-7256

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A technique for obtaining information on the temperature structure of a stellar atmosphere from spectral line data where only flux observations are available is discussed. The direct inversion of the flux integral to obtain the line source function can be circumvented by making the physically plausi