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Stellar Atmospheres: Beyond Classical Models

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Cover of 'Stellar Atmospheres: Beyond Classical Models'

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
Attention for Chapter 39: Formation of the K I 7699 Å Line in Sunspots
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Chapter title
Formation of the K I 7699 Å Line in Sunspots
Chapter number 39
Book title
Stellar Atmospheres: Beyond Classical Models
Published by
Springer, Dordrecht, January 1991
DOI 10.1007/978-94-011-3554-2_39
Book ISBNs
978-9-40-105574-1, 978-9-40-113554-2
Authors

B. Caccin, M. Carlsson, M. T. Gomez, G. Severino

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 1 Mendeley reader of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
United States 1 100%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 1 100%
Readers by discipline Count As %
Physics and Astronomy 1 100%