Francis Leblanc

An Introduction to Stellar Astrophysics

• Broschiertes Buch

Produktdetails

• Verlag: John Wiley & Sons Inc
• 2. Auflage
• Seitenzahl: 350
• Erscheinungstermin: 23. Oktober 2025
• Englisch
• ISBN-13: 9781394251797
• ISBN-10: 1394251793
• Artikelnr.: 73871874

Inhaltsangabe

Preface xi Acknowledgments xiii Chapter 1: Basic Concepts 1 1.1 Introduction 1 1.2 The Electromagnetic Spectrum 3 1.3 Blackbody Radiation 5 1.4 Luminosity, Effective Temperature, Flux and Magnitudes 8 1.5 Boltzmann and Saha Equations 13 1.6 Spectral Classification of Stars 21 1.7 The Hertzsprung-Russell Diagram 27 1.8 Summary 30 1.9 Exercises 31 Chapter 2: Stellar Formation 35 2.1 Introduction 35 2.2 Hydrostatic Equilibrium 36 2.3 The Virial Theorem 40 2.4 The Jeans Criterion 46 2.5 Free-Fall Times
52 2.6 Pre-Main-Sequence Evolution
54 2.7 Summary 57 2.8 Exercises 57 Chapter 3: Radiative Transfer in Stars 61 3.1 Introduction 61 3.2 Radiative Opacities 62 3.2.1 Matter-Radiation Interactions 62 3.2.2 Types of Radiative Opacities 64 3.3 Specific Intensity and Radiative Moments 69 3.4 Radiative Transfer Equation 77 3.5 Local Thermodynamic Equilibrium 81 3.6 Solution of the Radiative-Transfer Equation 82 3.7 Radiative Equilibrium 90 3.8 Radiative Transfer at Large Optical Depths 91 3.9 Rosseland and Other Mean Opacities 94 3.10 Schwarzschild-Milne Equations
97 3.11 Demonstration of the Radiative-Transfer Equation
99 3.12 Radiative Acceleration of Matter and Radiative Pressure
100 3.12.1 Radiative Acceleration of Matter 100 3.12.2 Radiative Pressure 103 3.13 Summary 104 3.14 Exercises 105 Chapter 4: Stellar Atmospheres 109 4.1 Introduction 109 4.2 The Grey Atmosphere 110 4.2.1 The Temperature Profile in a Grey Atmosphere 111 4.2.2 Radiative Flux in a Grey Atmosphere
117 4.3 Line Opacities and Broadening 119 4.3.1 Natural Broadening 120 4.3.2 Doppler Broadening 122 4.3.3 Pressure Broadening 130 4.3.4 Stimulated Emission and Masers 132 4.3.5 Einstein Coefficients
134 4.4 Equivalent Width and Formation of Atomic Lines 137 4.4.1 Equivalent Width 137 4.4.2 Formation of Weak Atomic Lines 139 4.4.3 Curve of Growth
142 4.5 Atmospheric Modelling 143 4.5.1 Input Data and Approximations 143 4.5.2 Algorithm for Atmospheric Modelling
145 4.5.3 Example of a Stellar Atmosphere Model 148 4.5.4 Temperature-Correction Procedure
150 4.6 Summary 151 4.7 Exercises 152 Chapter 5: Stellar Interiors 155 5.1 Introduction 155 5.2 Equations of Stellar Structure 156 5.2.1 Hydrostatic Equilibrium Equation 156 5.2.2 Equation of Mass Conservation 156 5.2.3 Energy-Transport Equation 159 5.2.4 Equation of Energy Conservation 160 5.2.5 Other Ingredients Needed 161 5.3 Energy Transport in Stars 163 5.3.1 Monochromatic Radiative Flux in Stellar Interiors 164 5.3.2 Conduction 166 5.3.3 Convection 167 5.3.3.1 General Description of Convection 167 5.3.3.2 The Schwarzschild Criterion for Convection
168 5.3.3.3 The Mixing-Length Theory
172 5.3.3.4 Convective Equilibrium
176 5.4 Polytropic Models 176 5.5 Structure of the Sun 182 5.6 Equation of State 184 5.6.1 Introduction 184 5.6.2 The Ideal Gas 185 5.6.3 Degeneracy 189 5.6.4 Radiation Pressure 191 5.7 Variable Stars and Asteroseismology 191 5.7.1 Variable Stars 191 5.7.2 Asteroseismology
197 5.7.3 Basic Physics Behind Period-Luminosity Relations
200 5.8 Summary 202 5.9 Exercises 203 Chapter 6: Nucleosynthesis and Stellar Evolution 205 6.1 Introduction 205 6.2 Generalities Concerning Nuclear Fusion 206 6.3 Models of the Nucleus
211 6.3.1 The Liquid-Drop Model 211 6.3.2 The Shell Model 214 6.4 Basic Physics of Nuclear Fusion 216 6.5 Main-Sequence Burning 218 6.5.1 Proton-Proton Chains 220 6.5.2 CNO Cycles 221 6.5.3 Lifetime of Stars on the Main Sequence 224 6.5.4 The Solar Neutrino Problem
226 6.6 Helium-Burning Phase 230 6.7 Advanced Nuclear Burning 232 6.7.1 Carbon-Burning Phase 233 6.7.2 Neon-Burning Phase 234 6.7.3 Oxygen-Burning Phase 234 6.7.4 Silicon-Burning Phase 235 6.8 Evolutionary Tracks in the H-R Diagram 236 6.8.1 Generalities 236 6.8.2 Evolution of Low-Mass Stars (M*
0.5 M
) 240 6.8.3 Evolution of a 1 M
Star: Our Sun 241 6.8.4 Evolution of Massive Stars (M*
10 M
) 245 6.9 Stellar Clusters 248 6.9.1 Stellar Populations, Galaxies and the Milky Way 248 6.9.2 Open Clusters 251 6.9.3 Globular Clusters 252 6.9.4 Age of Stellar Clusters 253 6.9.5 Distance to Stars and Stellar Clusters 255 6.10 Stellar Remnants 257 6.10.1 White Dwarfs 257 6.10.2 Neutron Stars, Pulsars and Magnetars 259 6.10.3 Black Holes 262 6.11 Novae and Supernovae
268 6.12 Heavy Element Nucleosynthesis: s, r and p Processes
273 6.12.1 The Slow and Rapid Processes 273 6.12.2 The p Process 276 6.13 Nuclear Reaction Cross Sections and Rates
277 6.14 Summary 281 6.15 Exercises 281 Chapter 7: Chemically Peculiar Stars and Diffusion
285 7.1 Introduction and Historical Background 285 7.2 Chemically Peculiar Stars 287 7.2.1 Am Stars 288 7.2.2 Ap Stars 288 7.2.3 HgMn Stars 289 7.2.4 He-Abnormal Stars 289 7.3 Atomic Diffusion Theory
290 7.4 Radiative Accelerations
297 7.5 Other Transport Mechanisms
302 7.5.1 Light-Induced Drift 303 7.5.2 Ambipolar Diffusion of Hydrogen 304 7.6 Summary 305 7.7 Exercises 305 Answers to Selected Exercises 307 Appendix A: Physical Constants 309 Appendix B: Units in the cgs and SI Systems 311 Appendix C: Astronomical Constants 313 Appendix D: Ionisation Energies (in eV) for the First Five Stages of Ionisation for the Most Important Elements 315 Appendix E: Solar Abundances for the Most Important Elements 317 Appendix F: Atomic Masses 319 Appendix G: Physical Parameters for Main-Sequence Stars 321 Appendix H: Periodic Table of the Elements 323 References 325 Bibliography 327 Index 329

Rezensionen

"An Introduction to Stellar Astrophysics is a welcome addition to existing books on this subject . . . Overall, a very good book. Summing Up: Recommended. Upper-division undergraduates, graduate students, and researchers/faculty." (Choice, 1July 2011)