R. Buccheri, J. van Paradijs, M. A. Alpar, The Many of Neutron Stars |
| |
Authors: | A C Fabian |
| |
Institution: | (1) Institute of Astronomy, Cambridge, U.K |
| |
Abstract: | We see neutron stars principally by their radio and X-ray emission. Their appearance in these different bands depends on whether
the emission comes from the surface or its magnetosphere. New phenomena continue to be found from neutron stars, which makes
it an exciting and topical research area. This volume is a collection of the papers from a NATO Advanced Study Institute held
in Italy in October 1996. Many, and for me the most interesting ones, are substantial reviews on topics such as Pulsar magnetic
fields and glitches (M. Ruderman), Radio pulsar population properties (D. Lorimer), Gamma-ray emission from CGRO pulsars (G.
Kanbach), Neutron stars and black holes in X-ray binaries (J. van Paradijs), Kilohertz quasi-periodic oscillations in low-mass
X-ray binaries (M. van der Klis), Thermonuclear burning on rapidly accreting neutron stars (L. Bildsten), On the X-ray emission
properties of rotation powered pulsars (W. Becker and J. Truemper). It will serve as a useful reference and source book for
students in high energy astrophysics and related fields. The high price may deter its purchase by individuals, but it will
be a good volume for a library needing recent coverage on neutron stars. It does not of course include the most recent developments
on anomalous X-ray pulsars or magnetars.
This revised version was published online in August 2006 with corrections to the Cover Date. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|