The third edition of this well-established textbook is ideal for advanced undergraduate and beginning graduate courses in high energy astrophysics. Now consolidated into a single-volume treatment, this textbook has been completely rewritten, providing a strong astronomical and astrophysical background for students to explore more advanced topics.
The third edition of this well-established textbook is ideal for advanced undergraduate and beginning graduate courses in high energy astrophysics. Now consolidated into a single-volume treatment, this textbook has been completely rewritten, providing a strong astronomical and astrophysical background for students to explore more advanced topics.
Malcolm S. Longair is Emeritus Jacksonian Professor of Natural Philosophy and Director of Development at the Cavendish Laboratory, University of Cambridge. He has held many senior positions in physics and astronomy, and has served on and chaired many national and international committees, boards and panels, working with both NASA and the European Space Agency. He has received much recognition for his work, including a CBE in the millennium honours list for his services to astronomy and cosmology. He is a Fellow of the Royal Society of London, the Royal Society of Edinburgh, the Academia Lincei and the Istituto Veneto di Scienze, Arte e Literatura.
Inhaltsangabe
Part I. Astronomical Background: 1. High energy astrophysics - an introduction; 2. The stars and stellar evolution; 3. The galaxies; 4. Clusters of galaxies; Part II. Physical Processes: 5. Ionisation losses; 6. Radiation of accelerated charged particles and bremsstrahlung of electrons; 7. The dynamics of charged particles in magnetic fields; 8. Synchrotron radiation; 9. Interactions of high energy photons; 10. Nuclear interactions; 11. Aspects of plasma physics and magnetohydrodynamics; Part III. High Energy Astrophysics in our Galaxy: 12. Interstellar gas and magnetic fields; 13. Dead stars; 14. Accretion power in astrophysics; 15. Cosmic rays; 16. The origin of cosmic rays in our galaxy; 17. The acceleration of high energy particles; Part IV. Extragalactic High Energy Astrophysics: 18. Active galaxies; 19. Black holes in the nuclei of galaxies; 20. The vicinity of the black hole; 21. Extragalactic radio sources; 22. Compact extragalactic sources and superluminal motions; 23. Cosmological aspects of high energy astrophysics; Appendix; References; Index.
Part I. Astronomical Background: 1. High energy astrophysics - an introduction; 2. The stars and stellar evolution; 3. The galaxies; 4. Clusters of galaxies; Part II. Physical Processes: 5. Ionisation losses; 6. Radiation of accelerated charged particles and bremsstrahlung of electrons; 7. The dynamics of charged particles in magnetic fields; 8. Synchrotron radiation; 9. Interactions of high energy photons; 10. Nuclear interactions; 11. Aspects of plasma physics and magnetohydrodynamics; Part III. High Energy Astrophysics in our Galaxy: 12. Interstellar gas and magnetic fields; 13. Dead stars; 14. Accretion power in astrophysics; 15. Cosmic rays; 16. The origin of cosmic rays in our galaxy; 17. The acceleration of high energy particles; Part IV. Extragalactic High Energy Astrophysics: 18. Active galaxies; 19. Black holes in the nuclei of galaxies; 20. The vicinity of the black hole; 21. Extragalactic radio sources; 22. Compact extragalactic sources and superluminal motions; 23. Cosmological aspects of high energy astrophysics; Appendix; References; Index.
Rezensionen
'The third edition of Malcolm Longair's High Energy Astrophysics is a remarkable gem. It is written in the clear, lucid style that characterizes Professor Longair's monographs and displays an admirable balance between breadth and depth. It is remarkably up to date and covers both high-energy phenomenology and physical processes with authority. It would serve equally well as a textbook for a graduate-level course or a reference work for the practising astrophysicist: a nicely written and sophisticated appendix on basic astronomy will make it equally useful for readers trained as physicists.' Bradley M. Peterson, Professor and Chair of Astronomy, Ohio State University
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