An Introduction to Modern Astrophysics

Höfundar: Bradley W. Carroll; Dale A. Ostlie (Útgáfa: 2)
An Introduction to Modern Astrophysics

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An Introduction to Modern Astrophysics is a comprehensive, well-organized and engaging text covering every major area of modern astrophysics, from the solar system and stellar astronomy to galactic and extragalactic astrophysics, and cosmology. Designed to provide students with a working knowledge of modern astrophysics, this textbook is suitable for astronomy and physics majors who have had a first-year introductory physics course with calculus.

Featuring a brief summary of the main scientific discoveries that have led to our current understanding of the universe; worked examples to facilitate the understanding of the concepts presented in the book; end-of-chapter problems to practice the skills acquired; and computational exercises to numerically model astronomical systems, the second edition of An Introduction to Modern Astrophysics is the go-to textbook for learning the core astrophysics curriculum as well as the many advances in the field.

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Útgefandi
Cambridge University Press
ISBN
9781108390248
Print ISBN
9781108422161
Format
Page Fidelity (PDF)
Útgáfa
2
Höfundar
Bradley W. Carroll; Dale A. Ostlie
Tungumál
English
Útgefið
2017-09-07
Prent takmörkun á líftíma
10

Kaflar

  • Half-title page
  • Title page
  • Copyright page
  • Dedication
  • Contents
  • Preface
  • Part I The Tools of Astronomy
  • 1 The Celestial Sphere
  • 1.1 The Greek Tradition
  • 1.2 The Copernican Revolution
  • 1.3 Positions on the Celestial Sphere
  • 1.4 Physics and Astronomy
  • 2 Celestial Mechanics
  • 2.1 Elliptical Orbits
  • 2.2 Newtonian Mechanics
  • 2.3 Kepler’s Laws Derived
  • 2.4 The Virial Theorem
  • 3 The Continuous Spectrum of Light
  • 3.1 Stellar Parallax
  • 3.2 The Magnitude Scale
  • 3.3 TheWave Nature of Light
  • 3.4 Blackbody Radiation
  • 3.5 The Quantization of Energy
  • 3.6 The Color Index
  • 4 The Theory of Special Relativity
  • 4.1 The Failure of the Galilean Transformations
  • 4.2 The Lorentz Transformations
  • 4.3 Time and Space in Special Relativity
  • 4.4 Relativistic Momentum and Energy
  • 5 The Interaction of Light and Matter
  • 5.1 Spectral Lines
  • 5.2 Photons
  • 5.3 The Bohr Model of the Atom
  • 5.4 Quantum Mechanics andWave–Particle Duality
  • 6 Telescopes
  • 6.1 Basic Optics
  • 6.2 Optical Telescopes
  • 6.3 Radio Telescopes
  • 6.4 Infrared, Ultraviolet, X-ray, and Gamma-Ray Astronomy
  • 6.5 All-Sky Surveys and Virtual Observatories
  • Part II The Nature of Stars
  • 7 Binary Systems and Stellar Parameters
  • 7.1 The Classification of Binary Stars
  • 7.2 Mass Determination Using Visual Binaries
  • 7.3 Eclipsing, Spectroscopic Binaries
  • 7.4 The Search for Extrasolar Planets
  • 8 The Classification of Stellar Spectra
  • 8.1 The Formation of Spectral Lines
  • 8.2 The Hertzsprung–Russell Diagram
  • 9 Stellar Atmospheres
  • 9.1 The Description of the Radiation Field
  • 9.2 Stellar Opacity
  • 9.3 Radiative Transfer
  • 9.4 The Transfer Equation
  • 9.5 The Profiles of Spectral Lines
  • 10 The Interiors of Stars
  • 10.1 Hydrostatic Equilibrium
  • 10.2 Pressure Equation of State
  • 10.3 Stellar Energy Sources
  • 10.4 Energy Transport and Thermodynamics
  • 10.5 Stellar Model Building
  • 10.6 The Main Sequence
  • 11 The Sun
  • 11.1 The Solar Interior
  • 11.2 The Solar Atmosphere
  • 11.3 The Solar Cycle
  • 12 The Interstellar Medium and Star Formation
  • 12.1 Interstellar Dust and Gas
  • 12.2 The Formation of Protostars
  • 12.3 Pre-Main-Sequence Evolution
  • 13 Main Sequence and Post-Main-Sequence Stellar Evolution
  • 13.1 Evolution on the Main Sequence
  • 13.2 Late Stages of Stellar Evolution
  • 13.3 Stellar Clusters
  • 14 Stellar Pulsation
  • 14.1 Observations of Pulsating Stars
  • 14.2 The Physics of Stellar Pulsation
  • 14.3 Modeling Stellar Pulsation
  • 14.4 Nonradial Stellar Pulsation
  • 14.5 Helioseismology and Asteroseismology
  • 15 The Fate of Massive Stars
  • 15.1 Post-Main-Sequence Evolution of Massive Stars
  • 15.2 The Classification of Supernovae
  • 15.3 Core-Collapse Supernovae
  • 15.4 Gamma-Ray Bursts
  • 15.5 Cosmic Rays
  • 16 The Degenerate Remnants of Stars
  • 16.1 The Discovery of Sirius B
  • 16.2 White Dwarfs
  • 16.3 The Physics of Degenerate Matter
  • 16.4 The Chandrasekhar Limit
  • 16.5 The Cooling of White Dwarfs
  • 16.6 Neutron Stars
  • 16.7 Pulsars
  • 17 General Relativity and Black Holes
  • 17.1 The General Theory of Relativity
  • 17.2 Intervals and Geodesics
  • 17.3 Black Holes
  • 18 Close Binary Star Systems
  • 18.1 Gravity in a Close Binary Star System
  • 18.2 Accretion Disks
  • 18.3 A Survey of Interacting Binary Systems
  • 18.4 White Dwarfs in Semidetached Binaries
  • 18.5 Type Ia Supernovae
  • 18.6 Neutron Stars and Black Holes in Binaries
  • Part III The Solar System
  • 19 Physical Processes in the Solar System
  • 19.1 A Brief Survey
  • 19.2 Tidal Forces
  • 19.3 The Physics of Atmospheres
  • 20 The Terrestrial Planets
  • 20.1 Mercury
  • 20.2 Venus
  • 20.3 Earth
  • 20.4 The Moon
  • 20.5 Mars
  • 21 The Realms of the Giant Planets
  • 21.1 The Giant Worlds
  • 21.2 The Moons of the Giants
  • 21.3 Planetary Ring Systems
  • 22 Minor Bodies of the Solar System
  • 22.1 Pluto and Charon
  • 22.2 Comets and Kuiper Belt Objects
  • 22.3 Asteroids
  • 22.4 Meteorites
  • 23 Formation of Planetary Systems
  • 23.1 Characteristics of Extrasolar Planetary Systems
  • 23.2 Planetary System Formation and Evolution
  • Part IV Galaxies and the Universe
  • 24 The MilkyWay Galaxy
  • 24.1 Counting the Stars in the Sky
  • 24.2 The Morphology of the Galaxy
  • 24.3 The Kinematics of the MilkyWay
  • 24.4 The Galactic Center
  • 25 The Nature of Galaxies
  • 25.1 The Hubble Sequence
  • 25.2 Spiral and Irregular Galaxies
  • 25.3 Spiral Structure
  • 25.4 Elliptical Galaxies
  • 26 Galactic Evolution
  • 26.1 Interactions of Galaxies
  • 26.2 The Formation of Galaxies
  • 27 The Structure of the Universe
  • 27.1 The Extragalactic Distance Scale
  • 27.2 The Expansion of the Universe
  • 27.3 Clusters of Galaxies
  • 28 Active Galaxies
  • 28.1 Observations of Active Galaxies
  • 28.2 A Unified Model of Active Galactic Nuclei
  • 28.3 Radio Lobes and Jets
  • 28.4 Using Quasars to Probe the Universe
  • 29 Cosmology
  • 29.1 Newtonian Cosmology
  • 29.2 The Cosmic Microwave Background
  • 29.3 Relativistic Cosmology
  • 29.4 Observational Cosmology
  • 30 The Early Universe
  • 30.1 The Very Early Universe and Inflation
  • 30.2 The Origin of Structure
  • Appendix C Solar System Data
  • Appendix D The Constellations
  • Appendix E The Brightest Stars
  • Appendix F The Nearest Stars
  • Appendix G Stellar Data
  • Appendix H The Messier Catalog
  • Appendix I Constants, A Programming Module
  • Appendix J Orbit, A Planetary Orbit Code
  • Appendix K TwoStars, A Binary Star Code
  • Appendix L StatStar, A Stellar Structure Code
  • Appendix M Galaxy, A Tidal Interaction Code
  • Appendix N WMAP Data
  • Suggested Reading
  • Index