X-ray Binaries (Cambridge Astrophysics)

 
Citation
Title:
X-ray Binaries (Cambridge Astrophysics)
Author:
Editor:
City:
Publisher:
Cambridge University Press
Year:
1997
Volume:
No. of Volumes:
Edition:
New Ed edition
Pages:
674
Series Volume:
Series Editor:
Series Title:
NATO ASI series. Series C, Mathematical and physical sciences ;
Translator:
Language:
English
URL:
DOI:
LCCN:
85030124
OCLC Number:
License
Select License
ISBN:
0521599342
9780521599344
Last Updated:
November 9th, 2011
Abstract

-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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