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Preface | p. vii |
A Message | p. ix |
Radiative Transfer and Model Atmospheres | |
From Complete Linearization to ALI and Beyond | p. 3 |
Quantitative Spectral Analysis of Evolved Low-Mass Stars | p. 15 |
The Second Stellar Spectrum and the Non-LTE Problem of the 2nd Kind | p. 27 |
Including All the Lines | p. 43 |
Accuracy of Stellar Opacities and the Solar Abundance Problem | p. 52 |
Particle Diffusion, Flows, and NLTE Calculations | p. 61 |
Quantitative Spectroscopy in 3D | p. 73 |
NLTE Model Atmospheres for Super-Soft X-ray Sources | p. 85 |
1D and 3D Radiative Transfer in Circumstellar Disks | p. 93 |
Hydrogen Lines in DA White Dwarfs: Improved Stark Broadening | p. 101 |
Stellar Winds | |
Radiation Driven Stellar Winds | p. 111 |
Mass Loss from OB-Stars | p. 123 |
Spectroscopy and Hydrodynamics of Dense Stellar Winds | p. 136 |
3D Radiative Transfer with PHOENIX | p. 148 |
Multi-dimensional Radiation Transport in Rapidly Expanding Envelopes | p. 161 |
Radiation Hydrodynamics of Line-driven Winds | p. 173 |
The Zeeman Effect in Hot-Star Winds with a Split Monopole Magnetic Field | p. 187 |
Time-dependent Non-LTE Radiative Transfer of Supernova Ejecta | p. 199 |
3D Non-LTE Time-dependent Spectrum Synthesis for Type Ia Supernovae | p. 207 |
Radiation Hydrodynamics | |
Radiation Hydrodynamics with Dimitri, ZEUS, and Athena | p. 217 |
Toward a Fully Consistent Radiation Hydrodynamics | p. 230 |
Accurate Radiation Hydrodynamics and MHD Modeling of 3-D Stellar Atmospheres | p. 242 |
Cosmological Radiation Hydrodynamics with Enzo | p. 260 |
Core-Collapse Supernova Explosion Simulations: The Path to and Necessity for 3D Models | p. 273 |
Self-consistent Thermodynamics in Accretion: Radiation-dominated Disks Are Thermally Stable | p. 284 |
Radiation-driven Outflows in Active Galactic Nuclei | p. 295 |
The Formation of Narrow X-ray Line Spectra from Realistic Hydrodynamical Models: Applications to the Problem of Warm Absorbers | p. 304 |
Photon Scattering in 3D Radiative MHD Simulations | p. 309 |
Radiative MHD Simulations of Sunspot Structure-Challenges and Recent Developments | p. 315 |
Teff and Log g Dependence of Velocity Fields in M-Stars | p. 323 |
RMHS Modeling of Solar Prominences | p. 331 |
Poster Session | |
Spectral Modeling of Accretion Disks around Compact Stars | p. 341 |
Neutron Star Model Atmospheres | p. 343 |
Quantitative Analysis of the Spectra of Early B Stars with Ultrasharp Lines | p. 345 |
The Impact of Stellar UV Spectroscopy on Stellar Population Studies | p. 347 |
Hydrogenic Line Widths Produced by Energy Fluctuations in Stellar Atmospheres | p. 349 |
Surface Velocity Fields from Tidal Interactions | p. 353 |
Calculation of the Solar UV/EUV Spectrum in Spherical Symmetry | p. 355 |
Static Spherically Symmetric NLTE Model Atmospheres Near the Eddington Limit | p. 357 |
Radiative Transfer in Axial Symmetry | p. 359 |
Formation of Helium Lines in Solar Prominences | p. 361 |
Comptonized Fe K-lines in the X-ray Spectra of Low-Mass X-ray Binaries | p. 363 |
Group Photo | p. 365 |
Author Index | p. 367 |
Table of Contents provided by Ingram. All Rights Reserved. |
The New copy of this book will include any supplemental materials advertised. Please check the title of the book to determine if it should include any access cards, study guides, lab manuals, CDs, etc.
The Used, Rental and eBook copies of this book are not guaranteed to include any supplemental materials. Typically, only the book itself is included. This is true even if the title states it includes any access cards, study guides, lab manuals, CDs, etc.