Princeton University Press
Physics of the Interstellar and Intergalactic Medium
About this book
An essential resource for graduate students and astrophysicists
This is a comprehensive and richly illustrated textbook on the astrophysics of the interstellar and intergalactic medium—the gas and dust, as well as the electromagnetic radiation, cosmic rays, and magnetic and gravitational fields, present between the stars in a galaxy and also between galaxies themselves.
Topics include radiative processes across the electromagnetic spectrum; radiative transfer; ionization; heating and cooling; astrochemistry; interstellar dust; fluid dynamics, including ionization fronts and shock waves; cosmic rays; distribution and evolution of the interstellar medium; and star formation. While it is assumed that the reader has a background in undergraduate-level physics, including some prior exposure to atomic and molecular physics, statistical mechanics, and electromagnetism, the first six chapters of the book include a review of the basic physics that is used in later chapters. This graduate-level textbook includes references for further reading, and serves as an invaluable resource for working astrophysicists.
- Essential textbook on the physics of the interstellar and intergalactic medium
- Based on a course taught by the author for more than twenty years at Princeton University
- Covers radiative processes, fluid dynamics, cosmic rays, astrochemistry, interstellar dust, and more
- Discusses the physical state and distribution of the ionized, atomic, and molecular phases of the interstellar medium
- Reviews diagnostics using emission and absorption lines
- Features color illustrations and detailed reference materials in appendices
- Instructor's manual with problems and solutions (available only to teachers)
Author / Editor information
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Topics
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Frontmatter
i -
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Contents
vii -
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Preface
xvii -
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1. Introduction
1 -
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2. Collisional Processes
11 -
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3. Statistical Mechanics and Thermodynamic Equilibrium
22 -
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4. Energy Levels of Atoms and Ions
32 -
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5. Energy Levels of Molecules
38 -
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6. Spontaneous Emission, Stimulated Emission, and Absorption
53 -
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7. Radiative Transfer
63 -
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8. HI 21-cm Emission and Absorption
70 -
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9. Absorption Lines: The Curve of Growth
75 -
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10. Emission and Absorption by a Thermal Plasma
92 -
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11. Propagation of Radio Waves through the ISM
101 -
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12. Interstellar Radiation Fields
119 -
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13. Ionization Processes
127 -
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14. Recombination of Ions with Electrons
137 -
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15. Photoionized Gas
162 -
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16. Ionization in Predominantly Neutral Regions
182 -
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17. Collisional Excitation
190 -
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18. Nebular Diagnostics
203 -
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19. Radiative Trapping
219 -
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20. Optical Pumping
229 -
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21. Interstellar Dust: Observed Properties
235 -
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22. Scattering and Absorption by Small Particles
248 -
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23. Composition of Interstellar Dust
263 -
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24. Temperatures of Interstellar Grains
285 -
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25. Grain Physics: Charging and Sputtering
296 -
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26. Grain Dynamics
304 -
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27. Heating and Cooling of H II Regions
315 -
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28. The Orion H II Region
326 -
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29. HI Clouds: Observations
331 -
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30. H I Clouds: Heating and Cooling
337 -
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31. Molecular Hydrogen
344 -
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32. Molecular Clouds: Observations
357 -
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33. Molecular Clouds: Chemistry and Ionization
373 -
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34. Physical Processes in Hot Gas
381 -
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35. Fluid Dynamics
389 -
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36. Shock Waves
397 -
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37. Ionization/Dissociation Fronts
412 -
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38. Stellar Winds
422 -
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39. Effects of Supernovae on the ISM
429 -
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40. Cosmic Rays and Gamma Rays
440 -
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41. Gravitational Collapse and Star Formation: Theory
451 -
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42. Star Formation: Observations
465 -
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A. List of Symbols
473 -
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B. Physical Constants
476 -
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C. Summary of Radiative Processes
477 -
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D. Ionization Potentials (eV)
481 -
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E. Energy-Level Diagrams
482 -
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F. Collisional Rate Coefficients
496 -
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G. Semiclassical Atom
503 -
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H. Debye Length for a Plasma
505 -
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I. Heuristic Model for Ion–Electron Inelastic Scattering
506 -
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J. Virial Theorem
508 -
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Bibliography
511 -
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Index
529