A relaxation method for the computation of model stellar atmospheres
- 1 June 1969
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 4 (2) , 182-212
- https://doi.org/10.1007/bf00650951
Abstract
No abstract availableKeywords
This publication has 9 references indexed in Scilit:
- Statistical Equilibrium Model Atmospheres for Early-Type Stars. III. Hydrogen and Helium ContinuaThe Astrophysical Journal, 1968
- Statistical-Equilibrium Model Atmospheres for Early-Type Stars. II. Formation of the Lyman ContinuumThe Astrophysical Journal, 1967
- Departures from LTE in g- and k- Star AtmospheresThe Astrophysical Journal, 1967
- Statistical-Equilibrium Model Atmospheres for Early-Type Stars. I. Hydrogen ContinuaThe Astrophysical Journal, 1967
- Deviations from LTE in stellar atmospheresJournal of Quantitative Spectroscopy and Radiative Transfer, 1966
- A statistical procedure for computing line-blanketed model stellar atmospheres with applications to the F5 IV star procyonJournal of Quantitative Spectroscopy and Radiative Transfer, 1966
- The Effect of Departures from LTE on the Stellar Continuum Fluxes in the Spectral-Type Range B5-A0The Astrophysical Journal, 1966
- Stark Broadening of Higher Hydrogen and Hydrogen-Like Lines by Electrons and Ions.The Astrophysical Journal, 1960
- The Hydrogen Emission in Gaseous NebulæMonthly Notices of the Royal Astronomical Society, 1932