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Line Blanketing in Real Stellar Atmospheres

Published online by Cambridge University Press:  07 February 2017

P. L. Bernacca
P. L. Bernacca*
Affiliation:
Asiago Observatory, Italy

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 146 - 148
Copyright
Copyright © Reidel 1973 

References

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