A statistical procedure for computing line-blanketed model stellar atmospheres with applications to the F5 IV star procyon
- 31 December 1966
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 6 (5), 591-607
- https://doi.org/10.1016/0022-4073(66)90048-3
Abstract
No abstract availableThis publication has 13 references indexed in Scilit:
- The Temperature Structure of Early-Type Model Stellar Atmospheres. II. a Grid of Stellar ModelsThe Astrophysical Journal Supplement Series, 1965
- A Model for a BI V Star with Line Blanketing.The Astrophysical Journal, 1965
- Oscillator Strengths for Lines of NiI.Journal of Research of the National Bureau of Standards Section A: Physics and Chemistry, 1965
- Oscillator Strengths for Lines of fe i Between 2500 and 3200 Å.The Astrophysical Journal, 1965
- Constant-Flux Convective Model Atmospheres.The Astrophysical Journal, 1965
- The Temperature Structure of Early-Type Model Stellar Atmospheres. I. Detailed Analysis of a 10000° K Model.The Astrophysical Journal, 1964
- On the Influence of the Chemical Composition on the Structure and Metal Index of Stellar Atmospheres.The Astrophysical Journal, 1964
- Absolute Oscillator Strengths for fe I.The Astrophysical Journal Supplement Series, 1964
- The Temperature Distribution in a Stellar Atmosphere.The Astrophysical Journal, 1963
- On the Effect of Fraunhofer Lines on u, b, V Measurements.The Astrophysical Journal, 1962