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Line Blanketing in Real Stellar Atmospheres
Published online by Cambridge University Press: 07 February 2017
Abstract
Ultraviolet observations of line blanketing in the spectrum variables α Scl and α2 CVn show that the usual procedure of allowing line blocking in model atmospheres has to be revised. It is also suggested that the region around 2900 Å could be safely used for determining effective temperatures.
- Type
- Part V: Ground Based and Extraterrestrial Observations of Stellar Flux
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- Copyright
- Copyright © Reidel 1973