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Stellar Atmospheres: Beyond Classical Models
Overview of attention for book
Table of Contents
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Book Overview
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Chapter 1
Recent Advances in Computational Methods
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Chapter 2
Acceleration of Convergence
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Chapter 3
Fast Solution of Radiative Transfer Problems with a Multi-Grid Method
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Chapter 4
Line Blanketing without LTE: Simple and Complex Spectra
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Chapter 5
Global and Local Methods for 1-D Problems; Implementation Aspects and CPU-Time and Memory Scalings
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Chapter 6
2-D Axisymmetric Line Transport
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Chapter 7
NLTE Spectral Line Formation in Three Dimensions
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Chapter 8
Iteration with Approximate Lambda Operators, and its Application to the Expanding Atmospheres of WR Stars
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Chapter 9
Analytical Methods of Line Formation Theory: Are they Still Alive?
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Chapter 10
Iteration Factors in the Solution of the NLTE Line Transfer Problem
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Chapter 11
Analysis of Ultraviolet P Cygni Profiles in the Spectra of O-Type Stars
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Chapter 12
Computer Codes for Stellar Atmospheric Modeling
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Chapter 13
The Quest for Physical Realism in Stellar Atmospheric Modeling
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Chapter 14
Unified NLTE Model Atmospheres Including Spherical Extension and Stellar Winds: EUV — Fluxes and the He II Discrepancy in Central Stars of Planetary Nebulae
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Chapter 15
Non-LTE Model Atmosphere Calculations with Approximate Lambda Operators
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Chapter 16
NLTE Model Atmospheres for Hot Stars
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Chapter 17
Radiative Transfer in Expanding Atmospheres — Radiative Acceleration of Wolf-Rayet Envelopes?
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Chapter 18
Non-LTE Analysis of Hot Stars Including Line Blanketing
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Chapter 19
Time-Dependent Two-Dimensional Radiation Hydrodynamics of Accreting Matter onto Highly Magnetized Neutron Stars: The Evolution of Photon Bubbles
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Chapter 20
The Origin and Development of Instabilities in Radiatively-Driven Stellar Winds
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Chapter 21
A Smooth Source Function Method for Including Scattering in Radiatively Driven Wind Simulations
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Chapter 22
2-D Radiation-Hydrodynamics Models of the Solar Photosphere
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Chapter 23
Dynamics of and Radiative Transfer in Inhomogeneous Media
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Chapter 24
Atmospheres of Late-Type Giants
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Chapter 25
FE II Emission Line Diagnostics of the Sun and Stars
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Chapter 26
Chromospheric Inhomogeneities in Cool Stars: Possible Effect on Hydrogen Line Profiles
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Chapter 27
Numerical Simulation of Photospheric Convection : Hydrodynamical Test Calculations
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Chapter 28
Stellar Atmosphere Theory as a Spectroscopic Tool. The Example of Hot Stars
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Chapter 29
The Winds of O-Stars V: Tests of the Accuracy of the Radiation Driven Wind Models
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Chapter 30
Diagnostics of Wolf-Rayet Atmospheres
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Chapter 31
Central Stars of PN: Spectral Diagnostics Based on Model Atmospheres vs. Diagnostics Based on the Classical Nebular Approach
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Chapter 32
Spectral Diagnostics of Hot Subdwarfs: Successes and Problems
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Chapter 33
Temperatures, Gravities and Abundances of B Stars: Recent Progress and Remaining Problems
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Chapter 34
Line Blanketing without LTE: The Effect on Diagnostics For B-Type Stars
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Chapter 35
Particle Transport in Magnetic Stellar Atmospheres
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Chapter 36
Spectroscopic Tests of Late-Type Model Atmospheres of Dwarf Stars
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Chapter 37
Dust in the Shells of Cool Giants and Supergiants
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Chapter 38
NLTE Analyses of Massive OB Stars
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Chapter 39
Formation of the K I 7699 Å Line in Sunspots
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Chapter 40
On the Influence of Multi-Dimensional Radiative Transfer on the Energetic Contribution of the Ca K Line
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Chapter 41
The Opacity Project and the Practical Utilization of Atomic Data
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Chapter 42
New Opacity Calculations
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Chapter 43
40 Years Numerical Stellar Atmospheres Concluding Remarks and Personal Considerations
Overall attention for this book and its chapters
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Mentioned by
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institution with syllabi
Citations
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Book overview
1. Recent Advances in Computational Methods
2. Acceleration of Convergence
3. Fast Solution of Radiative Transfer Problems with a Multi-Grid Method
4. Line Blanketing without LTE: Simple and Complex Spectra
5. Global and Local Methods for 1-D Problems; Implementation Aspects and CPU-Time and Memory Scalings
6. 2-D Axisymmetric Line Transport
7. NLTE Spectral Line Formation in Three Dimensions
8. Iteration with Approximate Lambda Operators, and its Application to the Expanding Atmospheres of WR Stars
9. Analytical Methods of Line Formation Theory: Are they Still Alive?
10. Iteration Factors in the Solution of the NLTE Line Transfer Problem
11. Analysis of Ultraviolet P Cygni Profiles in the Spectra of O-Type Stars
12. Computer Codes for Stellar Atmospheric Modeling
13. The Quest for Physical Realism in Stellar Atmospheric Modeling
14. Unified NLTE Model Atmospheres Including Spherical Extension and Stellar Winds: EUV — Fluxes and the He II Discrepancy in Central Stars of Planetary Nebulae
15. Non-LTE Model Atmosphere Calculations with Approximate Lambda Operators
16. NLTE Model Atmospheres for Hot Stars
17. Radiative Transfer in Expanding Atmospheres — Radiative Acceleration of Wolf-Rayet Envelopes?
18. Non-LTE Analysis of Hot Stars Including Line Blanketing
19. Time-Dependent Two-Dimensional Radiation Hydrodynamics of Accreting Matter onto Highly Magnetized Neutron Stars: The Evolution of Photon Bubbles
20. The Origin and Development of Instabilities in Radiatively-Driven Stellar Winds
21. A Smooth Source Function Method for Including Scattering in Radiatively Driven Wind Simulations
22. 2-D Radiation-Hydrodynamics Models of the Solar Photosphere
23. Dynamics of and Radiative Transfer in Inhomogeneous Media
24. Atmospheres of Late-Type Giants
25. FE II Emission Line Diagnostics of the Sun and Stars
26. Chromospheric Inhomogeneities in Cool Stars: Possible Effect on Hydrogen Line Profiles
27. Numerical Simulation of Photospheric Convection : Hydrodynamical Test Calculations
28. Stellar Atmosphere Theory as a Spectroscopic Tool. The Example of Hot Stars
29. The Winds of O-Stars V: Tests of the Accuracy of the Radiation Driven Wind Models
30. Diagnostics of Wolf-Rayet Atmospheres
31. Central Stars of PN: Spectral Diagnostics Based on Model Atmospheres vs. Diagnostics Based on the Classical Nebular Approach
32. Spectral Diagnostics of Hot Subdwarfs: Successes and Problems
33. Temperatures, Gravities and Abundances of B Stars: Recent Progress and Remaining Problems
34. Line Blanketing without LTE: The Effect on Diagnostics For B-Type Stars
35. Particle Transport in Magnetic Stellar Atmospheres
36. Spectroscopic Tests of Late-Type Model Atmospheres of Dwarf Stars
37. Dust in the Shells of Cool Giants and Supergiants
38. NLTE Analyses of Massive OB Stars
39. Formation of the K I 7699 Å Line in Sunspots
40. On the Influence of Multi-Dimensional Radiative Transfer on the Energetic Contribution of the Ca K Line
41. The Opacity Project and the Practical Utilization of Atomic Data
42. New Opacity Calculations
43. 40 Years Numerical Stellar Atmospheres Concluding Remarks and Personal Considerations
Summary
Syllabi
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Utrecht University
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