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Article contents
Line profiles in expanding atmospheres
Published online by Cambridge University Press: 26 May 2016
Extract
The analysis of the UV resonance transitions of superionized species observed in early-type stars suggests the presence of a high temperature region and an outward flow of matter (Snow & Marlborough 1976).
- Type
- 7. OB Stellar Winds
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- Copyright
- Copyright © Kluwer 1994