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Astrophysics of the Diffuse Universe

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This is a 13 page mind map about Astrophysics of the Diffuse Universe. Astronomy. 
 
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Astrophysics of the Diffuse Universe
>>Note: The book is designed as an astrophysics textbook that provides a comprehensive introduction to the physics of Interstellar Matter. It is aimed primarily at those undertaking postgraduate courses, or those doing advanced projects as part of honors undergraduate courses in physics or astrophysics. It should also provide a handy reference to the field for astrophysics faculty and other researchers who are not necessarily experts in this particular subdiscipline. The objective of Astrophysics of the Diffuse Universe is to show how physics can be applied to the understanding and diagnosis of the phase structure, the physical conditions, and the chemical make-up and evolution of the interstellar medium. Consistent with the authors' lecture and course experience, here a systematic approach has been adopted to assist the development of the reader's insight into the physics underlying the subject.
  Useful Atomic Data
  Hydrogenic Spectra
  The Helium II Spectrum
  The Hydrogen Spectrum
  Collisional Excitation Data
  Ionization Potentials
  Abundances
  What Is the Diffuse Universe?
  Phases
  Observability
  Collisional Ionization Equilibrium
  Continuum and Recombination Line Processes
  Line Emission Processes
  Collisional Excitation
  Line Transfer Effects
  Photoionizing Shocks
  The Oxygen-Rich Supernova Remnants
  Radiative Properties of Fast Shocks
  Production of Photoionized Shock Precursors
  The Structure of Radiative Fast Shocks
  Narrow Line Regions in Active Galaxies
  The Theory of Photoionized Regions
  Parameters of Photoionized Regions
  Rotational Wave function Symmetry
  Introduction to Astrochemistry
  Thermal Phases of Diffuse Matter
  Physical Constants
  Interstellar Shocks
  Interstellar Dust
  Continuum Data
  Free-Free Emission
  Total Free-Free Emission
  Two-Photon Emission
  Cooling Plasmas
 Astrophysics of the Diffuse Universe. Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Line Emission Processes
  Atomic Spectra
  Resonance Lines
  Pure Recombination Lines
  Spectroscopic Notation
  Intercombination and Forbidden Lines
  Molecular Spectra
  Rotating Molecules
  The Rigid Linear Rotator
  The Nonrigid Linear Rotator
  Polyatomic Linear Rotators
  Vibrating Molecules
  Ro-Vibrational Spectra
  Electronic Molecular Spectra
  The Franck-Condon Principle
  Ro-Vib-Electronic Molecular Spectra
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Line Transfer Effects
  Resonance Line Transfer
  Resonance Line Absorption by Heavy Elements
  Absorption Line Studies of the ISM
  Line Transfer in Emission Resonance Lines
  Escape Probabilities
  Mean Transmission Probabilities
  Mean Escape Probabilities - Emissivities
  Nebula Line Transfer
  Line Transfer in the Lyman Series
  The Hi 21 cm Line
  Hi Observations of Disk Galaxies
  Fluorescent Processes
  The Bowen Mechanism
  Oi Fluorescence with
  H2 Fluorescence with
  Raman Scattering Fluorescence
  Astrophysical Masers
  Theory
  Observations of Galactic Masers
  Observations of Extragalactic Masers
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Thermal Phases of Diffuse Matter
  Phase Stability
  Thermal Phases of Galactic Interstellar Gas
  Giant Molecular Clouds
  The Atomic ISM
  Theoretical Phase Structure of the Atomic ISM
  Warm Ionized Phases
  The Hot Ionized Component
  Feedback and Mass Exchange
  Shells, Supershells, and Interstellar Froth
  Self-Propagating Star Formation
  Self-Regulated Star Formation
  Mass Exchange
  Dust Evolution in a Multiphase Medium
  Back to the Beginning: The Epoch of Galaxy Formation
  Star-Formation Rates in the Early Universe
  High-Redshift Radio Galaxies
  The Reionization Epoch
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 The Theory of Photoionized Regions
  Photoionization of Hydrogen Hii Regions
  Equilibrium Ionization Parameters
  The Diffuse Field: Case A and Case B
  Ionization Fronts
  Jump Conditions in Ionization Fronts
  Photoionization of Neutral Condensations
  Hii Regions with Heavy Elements
  Ionization Structure of Hydrogen and Helium Nebulae
  Nebular Structure with Heavy Elements
  Nebular Equilibrium Temperature
  Photoionization by X-ray Sources
  Radio Continuum of Hii Regions
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Interstellar Shocks
  Why Do Shocks Exist?
  J-Shocks
  The Rankine-Hugoniot Jump Conditions
  Radiationless Shocks
  Isothermal Shocks
  The Drivers of Interstellar Shocks
  Supernova Explosions
  Stellar Wind Bubbles
  Galactic Jet-Driven Bubbles
  The Radiative Properties of J-shocks
  Radiation Properties of Shock Fronts
  The Structure of Radiative J-Shocks
  Spectra of Old Supernova Remnants
  Spectra of Herbig-Haro Objects
  C-Shocks
  The Structure and Spectrum of C-Shocks
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
  Parameters of Photoionized Regions
  Nebular Parameters
  Nebular Temperature
  Ionized Masses and Densities
  Ionizing Source Parameters
  UV Flux Distribution
  Stellar Atmospheric Modelling
  Zanstra Temperatures
  Energy Balance (Stoy) Temperatures
  Photoionization Modelling
  Ionization Correction Factors
  Self-Consistent Photoionization Modelling
  Abundances
  Galactic Abundance Gradients from Hii Regions
  Abundances in Planetary Nebulae (PNe)
  Nova Shells
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Interstellar Dust
  Stardust Formation
  Grain Condensation in Oxygen-Rich Atmospheres
  Grain Condensation in Carbon-Rich Atmospheres
  Grain Photoheating
  Quantum Heating
  The Life Cycle of Grains
  Thermal Sputtering
  Grain-Grain Collisions
  The Optical Properties of Dust
  Extinction Definitions
  Optical Efficiency Factors
  Polarization by Dust
  Radiation Pressure Effects
  Spectral Signatures of Grain Materials
  Constraints from the Spectral Energy Distribution
  Silicates
  Icy Grain Mantles
  Polycyclic Aromatic Hydrocarbons (PAHs)
  The Survival of PAHs in the ISM
  The Diffuse Interstellar Bands (DIBs)
  Grain Charging
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Cooling Plasmas
  The Cooling Function
  Conditions for Nonequilibrium Cooling
  Heat Transport
  Electron Conduction
  Boundary Layer Mixing
  Cold Clouds in Hot Gas
  Thermal Instabilities
  In a Stationary Medium
  In an Expanding Medium
  The Recombination Era of the Universe
  Hot Galactic Coronae
  Early-Type Galaxies
  Clusters of Galaxies
  Disk Galaxies
 Astrophysics of the Diffuse Universe. Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Collisional Ionization Equilibrium
  Collisional Ionization
  The Case of Hydrogen
  Recombination
  Radiative Recombination Rates
  Dielectronic Recombination Rates
  Photoionization
  From Outer Shells
  Inner Shell Photoionization
  The Milne Relation
  Photoionization Cross Sections
  Charge-Exchange
  Coronal Equilibrium
  The Case of a Pure Hydrogen Plasma
  Ionization Equilibrium of Heavy Elements
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
  Introduction to Astrochemistry
  Molecular Formation and Destruction
  Neutral Gas-Phase Reactions
  Ion-Molecule Chemistry
  Dust-Grain Moderated Chemistry
  Molecular Destruction Processes
  Chemistry of Particular Regions
  Cold Molecular Clouds
  Photodissociation Regions
  Shock Chemistry
  Hot Molecular Cores
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Continuum and Recombination Line Processes
  Free-Free Continuum Emission
  Free-Free Gaunt Factors
  The Free-Bound Continuum
  Continuum Emission Coefficients
  The Two-Photon Process
  Recombination Line Emission
  Recombination Line Spectra
  The Radio Recombination Lines
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland
 >>New Map
 Collisional Excitation
  Collisional Excitation by Electron Impact
  Limiting Cases
  The Three-Level Atom
  Low-Density Limit
  Ions in Which
  Infrared Line Diagnostics
  The General Multilevel Atom
 Astrophysics of the Diffuse Universe
 Michael A.Dopita, Ralph S.Sutherland