A computer program for calculating non-LTE model stellar atmospheres

Computer Physics Communications

Volumn 52, Issue 1, 1988, Pages 103-132

  Hubeny, I ^a  

^a UNIVERSITY OF COLORADO   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0039617444     PISSN: 00104655     EISSN: None     Source Type: Journal    
DOI: 10.1016/0010-4655(88)90177-4     Document Type: Article

References (31)

1. Non-Lte Model Atmospheres. III. a Complete-Linearization Method
2. On the Use of Variable Eddington Factors in Non-LTE Stellar Atmospheres Computations
3. Frequency-Quadrature Perturbations in Radiative-Transfer Theory
4. Solutions to radiative transfer problems using approximate lambda operators
5. Line blanketing without local thermodynamic equilibrium. I - A hydrostatic stellar atmosphere with hydrogen, helium, and carbon lines
6. A Computer Program for Solving Multi-level Non-LTE Radiative Transfer Problems in Moving or Static Atmospheres
7. Photospheres of hot stars. I - Wind-blanketed model atmospheres
8. Radiative Transfer in Spherically Symmetric Systems-III: FUNDAMENTALS OF LINE FORMATION
9. Solution of the comoving-frame equation of transfer in spherically symmetric flows. V - Multilevel atoms
10. ATLAS: A Computer Program for Calculating Model Stellar Atmospheres
11. Photoionization Cross-Sections for Atoms and Ions of Carbon, Nitrogen, Oxygen, and Neon
12. Rate Coefficients for Electron Excitation of the First Resonance Transition in h, Li, Na, Ca, Ca', and Ba' Calculated from Experimental Data
13. Tabellen für Berechnung von Zustandsummen