W. Kluzniak
Published 2000-12-29Version 1
The basic observed properties of neutron stars are reviewed. I suggest that neutron stars in low-mass X-ray binaries are the best of all known sites for testing strong-field effects of general relativity.
Comments: Lectures given at the Mexican School of Astrophysics, Guanajuato, August 1999
Journal: From the Sun to the Great Attractor, D. Page, J.G. Hirsch eds., (2000), (Heidelberg:Springer) 173
The Zel'dovich-type approximation for an inhomogeneous universe in general relativity: second-order solutions
Solving the Problem of Time in General Relativity and Cosmology with Phantoms and k -- Essence
Galactic Dynamics via General Relativity: A Compilation and New Developments
