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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
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Title
Stellar Atmospheres: Beyond Classical Models
Published by
Springer Netherlands, December 2012
DOI 10.1007/978-94-011-3554-2
ISBNs
978-9-40-113554-2, 978-9-40-105574-1
Editors

Crivellari, L., Hummer, D. G., Hubeny, I.

Mendeley readers

The data shown below were compiled from readership statistics for 10 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 10 100%

Demographic breakdown

Readers by professional status Count As %
Researcher 4 40%
Student > Ph. D. Student 3 30%
Student > Master 2 20%
Unspecified 1 10%
Readers by discipline Count As %
Physics and Astronomy 8 80%
Agricultural and Biological Sciences 1 10%
Unspecified 1 10%