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Astrophysics of Neutron Stars

BuchKartoniert, Paperback
Verkaufsrang24739inPhysik und Astronomie
CHF109.00

Beschreibung

The existence of neutron stars was not only a brilliant theoretical prediction, but also one of the most unexpected and astonishing discoveries of all heavenly bodies. Twenty-five years after the remarkable event of their discovery, neutron stars, which are the densest, the most strongly magnetized, and the most rapid ly rotating bodies in the Galaxy, remain objects of intense interest. This book is a revised and enlarged version of the original Russian edition. The last five years were marked by the discovery of a supernova in the closest galaxy and dozens of X-ray sources and millisecond pulsars, which apparently confirm the validity of the basic ideas underlying these discoveries. The author has concentrated on the astrophysical manifestations of neutron stars, which are believed mainly to be associated with the nature of their interaction with their surroundings. Naturally, this approach does not leave much room for a detailed description of the internal structure of these stars. Fortunately, there exists an excellent monograph by S. L. Shapiro and S. A. Teukolsky (Black Holes, White Dwarfs, and Neutron Stars, Wiley, New York 1985) which deals mainly with the purely physical problems. Moreover, the publication of such a book in the West partly makes amends for the lack of information about the work being done by Soviet scientists in this field.
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Details

ISBN/GTIN978-3-642-76352-6
ProduktartBuch
EinbandKartoniert, Paperback
Erscheinungsdatum06.12.2011
AuflageSoftcover reprint of the original 1st ed. 1992
Seiten340 Seiten
SpracheEnglisch
MasseBreite 155 mm, Höhe 235 mm, Dicke 19 mm
Gewicht517 g
Artikel-Nr.14126208
KatalogBuchzentrum
Datenquelle-Nr.13332324
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Reihe

Über den/die AutorIn

In this book will be found a description of the current state of experimental and theoretical investigations of neutron stars in all their manifestations. The approach adopted leads to topics in plasma physics and magnetohydrodynamics also being discussed. Students and professionals in astrophysics and physics alike will find this revised and enlarged version of the original Russian edition essential reading for its coverage of neutron star classification and evolution.

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