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Theory of Neutron Star Magnetospheres (Theoretical Astrophysics)
 
 
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Theory of Neutron Star Magnetospheres (Theoretical Astrophysics) [Paperback]

Michel

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Product details

  • Paperback: 532 pages
  • Publisher: University of Chicago Press; illustrated edition edition (1 Nov 1990)
  • Language English
  • ISBN-10: 0226523314
  • ISBN-13: 978-0226523316
  • Product Dimensions: 2.3 x 1.5 x 0.3 cm
  • Amazon Bestsellers Rank: 5,622,364 in Books (See Top 100 in Books)

More About the Author

F. Curtis Michel
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Product Description

Product Description

An incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, "Theory of Neutron Star Magnetospheres" sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists faced with a huge and widely scattered literature.
F. Curtis Michel, who was among the first theorists to propose a neutron star model for radio pulsars, analyzes competing models of pulsars, radio emission models, winds and jets from pulsars, pulsating X-ray sources, gamma-ray burst sources, and other neutron-star driven phenomena. Although the book places primary emphasis on theoretical essentials, it also provides a considerable introduction to the observational data and its organization. Michel emphasizes the problems and uncertainties that have arisen in the research as well as the considerable progress that has been made to date.

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First Sentence
One of several important discoveries of recent years has been that of pulsars, astrophysical objects that produce sharp pulses of relatively low frequency radio emission of considerable intensity. Read the first page
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Front Cover | Copyright | Table of Contents | Excerpt | Index | Back Cover
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