X-Ray Binaries

X-Ray Binaries

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X-ray binaries are some of the most varied and perplexing systems known to astronomers. The compact object which accretes mass from its companion star may be a white dwarf, neutron star, or black hole, whereas the donor star can be a 'normal' star or a white dwarf. The various combinations differ widely in their behaviour, and this timely volume provides a unique reference of our knowledge to date of all of them. Fifteen specially written chapters by a team of the world's foremost researchers in the field explore all aspects of the X-ray binaries. They cover the X-ray, ultraviolet, optical and radio properties of these violent systems and address key issues such as: how were these systems formed, and what will be their fate; how can we understand X-ray bursts, and how the quasi-periodic oscillations; what is the connection between millisecond radio pulsars and low-mass X-ray binaries; and how does the magnetic field of a neutron star decay? This long awaited review provides graduate students and researchers with the standard reference on X-ray binaries for many years to come.

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  • Paperback | 676 pages
  • 175.3 x 247.1 x 30.5mm | 1,315.43g
  • CambridgeUnited Kingdom
  • English
  • Revised ed.
  • 21 b/w illus. 36 tables
  • 0521599342
  • 9780521599344
  • 1,385,926

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"This book will be a valuable addition to any physics or astronomy library; even the nonexpert will benefit from a few hours browsing through it." Herbert Gursky, American Scientist

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