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Addison-Wesley / Prentice Hall

Physics & Astronomy

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Introduction to Modern Astrophysics, An
Bradley W. CarrollWeber State University
Dale A. OstlieWeber State University

ISBN-10: 0201547309
ISBN-13:  9780201547306

Publisher:  Addison-Wesley
Copyright:  1996
Format:  Cloth; 1326 pp
Published:  12/11/1995

This exciting text opens the entire field of modern astrophysics to the reader by using only the basic tools of physics. Designed for the junior- level astrophysics course, each topic is approached in the context of the major unresolved questions in astrophysics. The core chapters have been designed for a course in stellar structure and evolution, while the extended chapters provide additional coverage of the solar system, galactic structure, dynamics, evolution, and cosmology.



This product accompanies:
Carroll & Ostlie,  Introduction to Modern Astrophysics, An, 2/E

  • Two versions of this text are available: An Introduction to Modern Stellar Astrophysics, (Chapters 1-17), and An Introduction to Modern Astrophysics, (Chapters 1-28).
  • Computer programs included with the text allow students to explore the physics of stars and galaxies.
  • In designing a curriculum, instructors can combine core and extended chapters with the optional advanced sections so as to meet their individual goals.
  • Up-to-date coverage of current astrophysical discoveries are included.
  • This text emphasizes computational physics, including computer problems and on-line programs.
  • This text also includes a selection of over 500 problems. For additional information and computer codes to be used in conjunction with the text, visit the astrophysics homepage at Weber State: http://astrophysics.weber.edu

I. TOOLS FOR ASTRONOMY.

 1. The Celestial Sphere.

 2. Celestial Mechanics.

 3. The Continuous Spectrum of Light.

 4. The Theory of Special Relativity.

 5. The Interaction of Light and Matter.

 6. Telescopes.

II. THE NATURE OF STARS.

 7. Binary Stars and Stellar Parameters.

 8. The Classification of Stellar Spectra.

 9. Stellar Atmospheres.

10. The Interiors of Stars.

11. The Sun.

12. The Process of Star Formation.

13. Post-Main-Sequence Stellar Evolution.

14. Stellar Pulsation.

15. The Degenerate Remnants of Stars.

16. Black Holes.

17. Close Binary Star Systems.

III. THE SOLAR SYSTEM.

18. Physical Processes in the Solar System.

19. The Terrestrial Planets.

20. The Jovian Worlds.

21. Pluto, Solar System Debris, and Formation.

IV. GALAXIES AND THE UNIVERSE.

22. The Milky Way Galaxy.

23. The Nature of Galaxies.

24. Galactic Evolution.

25. The Structure of the Universe.

26. Active Galaxies.

27. Cosmology.

28. The Early Universe.

Appendices.

Index.

  • 9780805304022
    Introduction to Modern Astrophysics, An, 2/E
    Carroll & Ostlie
    ©2007 | Addison-Wesley | Cloth; 1400 pp | Instock
    ISBN-10: 0805304029 | ISBN-13: 9780805304022
    Brief Description

Bradley Carroll received his B.A. in Mathematics and a Secondary Teaching Credential from the University of California, Irvine, his M.S. in Physics from the University of Colorado, Boulder and his Ph.D. Astrophysics from the University of Colorado, Boulder.

Brad's lifelong fascination with astronomy, combined with a happy naivete concerning what lay ahead, led him to graduate school at CU Boulder. His thesis, supervised by Carl Hansen and John Cox, was a study of the effect of rotation on pulsating stars. Brad then headed east to work as a postdoc with Hugh Van Horn at the University of Rochester, where he carried out research on the oscillations of accretion disks and neutron stars. At both CU Boulder and the U of R, he learned the virtues of making simple models of complex astrophysical systems. .

Four years later, as the postdoc came to an end, Brad was lucky to find a teaching position in the Physics Department at Weber State University, and doubly lucky that Dale Ostlie was there. It is rare to find two experts in Stellar pulsation in the same institution and department, especially when their outlooks are congenial. .

Brad truly enjoys teaching which gives him the chance to share the wonders of the physical world with his students. Such a background served him well (especially his naivete about what lay ahead) when he and Dale decided to write An Introduction to Modern Astrophysics. Now that the book and solutions manual, are completed, Brad once again has the time to enjoy traveling, camping, and fishing.


Dale A. Ostlie's long-time interest in astronomy began with his childhood fascination in the space program, including vivid recollections of watching the Apollo missions with his family. His interest in teaching was born from his experiences as a student, being fortunate to have had excellent instructors and mentors in high school, college, and graduate school. During graduate school, Dale had the opportunity to spend a significant period of time working with Dr. Arthur N. Cox and the theoretical astrophysics group at Los Alamos National Laboratory. While at Los Alamos, Dale was introduced to great number of exciting and challenging problems in astrophysics, which spurred his interest in developing a broad exposure to the discipline.

After completing his graduate thesis on Mira variable stars, and after a two-year teaching position at Bates College in Maine, Dale accepted a teaching position at Weber State University. With WSU nestled up against the Wasatch mountains of Utah, Dale is able to indulge his addictions to skiing, hiking, camping, and mountain biking. One year after Dale arrived at Weber State, Brad Carroll was hired, and their partnership in stellar pulsation studies and text-book writing was born. Sharing many of the same pedagogical views, as well as a dedication to producing the best possible text, Brad and Dale worked for six years to write An Introduction to Modern Stellar Astrophysics and An Introduction to Modern Astrophysics, and another year to produce the Instructor's Solutions Manual. Work related to the texts continues today with the maintenance of a collection of web pages associated with the books, including discussions of new discoveries since the publication of the texts in 1996.


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