Hostname: page-component-f554764f5-nqxm9 Total loading time: 0 Render date: 2025-04-17T01:46:11.065Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Bernacca, P. L. and Molnar, M. R.: 1972, Astrophys. J. 178, No. 1.CrossRefGoogle Scholar
Bradley, P. T. and Morton, D. C.: 1969, Astrophys. J. 156, 687.CrossRefGoogle Scholar
Klinglesmith, D. A.: 1971, NASA SP-3065.Google Scholar
Norris, J.: 1971, Astrophys. J. Suppl. 23, 213.CrossRefGoogle Scholar
Underhill, A. B.: 1971, Proceedings OAO-Symposium , Amherst, Mass., NASA-SP-310, 367.Google Scholar